Venus

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Venus

A real-colour image of Venus processed from two filters. The surface is obscured by a thick blanket of clouds.
Designations
Pronunciation	i/ˈviːnəs/
Adjectives	Venusian or (rarely) Cytherean, Venerean
Orbital characteristics[2][4]
Epoch J2000
Aphelion	0.728213 AU 108939000 km
Perihelion	0.718440 AU 107477000 km
Semi-major axis	0.723327 AU 108208000 km
Eccentricity	0.0067
Orbital period	224.701 d 0.615198 yr 1.92 Venus solar day
Synodic period	583.92 days[2]
Average orbital speed	35.02 km/s
Mean anomaly	50.115°
Inclination	3.39458° to ecliptic 3.86° to Sun's equator 2.19° to invariable plane[3]
Longitude of ascending node	76.678°
Argument of perihelion	55.186°
Satellites	None
Physical characteristics
Mean radius	6051.8±1.0 km[5] 0.9499 Earths
Flattening	0[5]
Surface area	4.60×108 km2 0.902 Earths
Volume	9.28×1011 km3 0.866 Earths
Mass	4.8676×1024 kg 0.815 Earths
Mean density	5.243 g/cm3
Surface gravity	8.87 m/s2 0.904 g
Escape velocity	10.36 km/s
Sidereal rotation period	−243.0185 d (retrograde)
Equatorial rotation velocity	6.52 km/h (1.81 m/s)
Axial tilt	177.36°[2]
North pole right ascension	18h 11m 2s 272.76°[6]
North pole declination	67.16°
Albedo	0.67 (geometric)[7] 0.90 (Bond)[7]
Surface temp. min mean max Kelvin 737 K[2] Celsius 462 °C
Apparent magnitude	brightest −4.9[8][9] (crescent) −3.8[10] (full)
Angular diameter	9.7″ to 66.0″[2]
Atmosphere
Surface pressure	92 bar (9.2 MPa)
Composition by volume	≈ 96.5% carbon dioxide ≈ 3.5% nitrogen 0.015% sulfur dioxide 0.007% argon 0.002% water vapour 0.0017% carbon monoxide 0.0012% helium 0.0007% neon trace carbonyl sulfide trace hydrogen chloride trace hydrogen fluoride

Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.^[11] It has no natural satellite. It is named after the Roman goddess of love and beauty. After the Moon, it is the brightest natural object in the night sky, reaching an apparent magnitude of −4.6, bright enough to cast shadows.^[12] Because Venus is an inferior planet from Earth, it never appears to venture far from the Sun: its elongation reaches a maximum of 47.8°.

Venus is a terrestrial planet and is sometimes called Earth's "sister planet" because of their similar size, mass, proximity to the Sun and bulk composition. However, it has also been shown to be radically different from Earth in other respects. It has the densest atmosphere of the four terrestrial planets, consisting of more than 96% carbon dioxide. The atmospheric pressure at the planet's surface is 92 times that of Earth's. With a mean surface temperature of 735 K (462 °C; 863 °F), Venus is by far the hottest planet in the Solar System, even though Mercury is closer to the Sun. Venus has no carbon cycle that puts carbon into rock, nor does it seem to have any organic life to absorb carbon in biomass. Venus is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light. It may have possessed oceans in the past,^[13][14] but these would have vaporized as the temperature rose due to a runaway greenhouse effect.^[15] The water has most probably photodissociated, and, because of the lack of a planetary magnetic field, the free hydrogen has been swept into interplanetary space by the solar wind.^[16] Venus' surface is a dry desertscape interspersed with slab-like rocks and periodically refreshed by volcanism.

Physical characteristics

Venus is one of the four terrestrial planets in the Solar System, meaning that, like Earth, it is a rocky body. In size and mass, it is similar to Earth, and is often described as Earth's "sister" or "twin".^[17] The diameter of Venus is 12,092 km (only 650 km less than Earth's) and its mass is 81.5% of Earth's. Conditions on the Venusian surface differ radically from those on Earth, owing to its dense carbon dioxide atmosphere. The mass of the atmosphere of Venus is 96.5% carbon dioxide, with most of the remaining 3.5% being nitrogen.^[18]

Geography

The Venusian surface was a subject of speculation until some of its secrets were revealed by planetary science in the 20th century. It was finally mapped in detail by Project Magellan in 1990–91. The ground shows evidence of extensive volcanism, and the sulfur in the atmosphere may indicate there have been some recent eruptions.^[19][20]

About 80% of the Venusian surface is covered by smooth, volcanic plains, consisting of 70% plains with wrinkle ridges and 10% smooth or lobate plains.^[21] Two highland "continents" make up the rest of its surface area, one lying in the planet's northern hemisphere and the other just south of the equator. The northern continent is called Ishtar Terra, after Ishtar, the Babylonian goddess of love, and is about the size of Australia. Maxwell Montes, the highest mountain on Venus, lies on Ishtar Terra. Its peak is 11 km above the Venusian average surface elevation. The southern continent is called Aphrodite Terra, after the Greek goddess of love, and is the larger of the two highland regions at roughly the size of South America. A network of fractures and faults covers much of this area.^[22]

The absence of evidence of lava flow accompanying any of the visible caldera remains an enigma. The planet has few impact craters, demonstrating the surface is relatively young, approximately 300–600 million years old.^[23][24] In addition to the impact craters, mountains, and valleys commonly found on rocky planets, Venus has some unique surface features. Among these are flat-topped volcanic features called "farra", which look somewhat like pancakes and range in size from 20 to 50 km across, and from 100 to 1,000 m high; radial, star-like fracture systems called "novae"; features with both radial and concentric fractures resembling spider webs, known as "arachnoids"; and "coronae", circular rings of fractures sometimes surrounded by a depression. These features are volcanic in origin.^[25]

Most Venusian surface features are named after historical and mythological women.^[26] Exceptions are Maxwell Montes, named after James Clerk Maxwell, and highland regions Alpha Regio, Beta Regio and Ovda Regio. The former three features were named before the current system was adopted by the International Astronomical Union, the body that oversees planetary nomenclature.^[27]

The longitudes of physical features on Venus are expressed relative to its prime meridian. The original prime meridian passed through the radar-bright spot at the center of the oval feature Eve, located south of Alpha Regio.^[28] After the Venera missions were completed, the prime meridian was redefined to pass through the central peak in the crater Ariadne.^[29][30]

Size comparison of Mercury, Venus, Earth and the Moon, Mars, and Ceres on the far right. This may not be exactly to scale, because the visual disc of Venus with its atmosphere makes it look bigger than its solid-body diameter.

Surface geology

Maat Mons with a vertical exaggeration of 22.5

Much of the Venusian surface appears to have been shaped by volcanic activity. Venus has several times as many volcanoes as Earth, and it possesses 167 large volcanoes that are over 100 km across. The only volcanic complex of this size on Earth is the Big Island of Hawaii.^[25] This is not because Venus is more volcanically active than Earth, but because its crust is older. Earth's oceanic crust is continually recycled by subduction at the boundaries of tectonic plates, and has an average age of about 100 million years,^[31] whereas the Venusian surface is estimated to be 300–600 million years old.^[23][25]

Several lines of evidence point to ongoing volcanic activity on Venus. During the Soviet Venera program, the Venera 11 and Venera 12 probes detected a constant stream of lightning, and Venera 12 recorded a powerful clap of thunder soon after it landed. The European Space Agency's Venus Express recorded abundant lightning in the high atmosphere.^[32] Although rainfall drives thunderstorms on Earth, there is no rainfall on the surface of Venus (though sulfuric acid rain falls in the upper atmosphere, then evaporates around 25 km above the surface). One possibility is that ash from a volcanic eruption was generating the lightning. Another piece of evidence comes from measurements of sulfur dioxide concentrations in the atmosphere, which dropped by a factor of 10 between 1978 and 1986. This may mean the levels had earlier been boosted by a large volcanic eruption.^[33] Almost a thousand impact craters on Venus are evenly distributed across its surface. On other cratered bodies, such as Earth and the Moon, craters show a range of states of degradation. On the Moon, degradation is caused by subsequent impacts, whereas on Earth it is caused by wind and rain erosion. On Venus, about 85% of the craters are in pristine condition. The number of craters, together with their well-preserved condition, indicates the planet underwent a global resurfacing event about 300–600 million years ago,^[23][24] followed by a decay in volcanism.^[34] Whereas Earth's crust is in continuous motion, Venus is thought to be unable to sustain such a process. Without plate tectonics to dissipate heat from its mantle, Venus instead undergoes a cyclical process in which mantle temperatures rise until they reach a critical level that weakens the crust. Then, over a period of about 100 million years, subduction occurs on an enormous scale, completely recycling the crust.^[25] In March 2014, the first direct evidence for ongoing volcanism was located, in the form of infrared "flashes" over the rift zone Ganiki Chasma, near the shield volcano Maat Mons. These flashes, ranging from 40 to 320 °C above the ambient, are believed to be either hot gases or lava released from volcanic eruptions.^[35]

Venusian craters range from 3 km to 280 km in diameter. No craters are smaller than 3 km, because of the effects of the dense atmosphere on incoming objects. Objects with less than a certain kinetic energy are slowed down so much by the atmosphere that they do not create an impact crater.^[36] Incoming projectiles less than 50 metres in diameter will fragment and burn up in the atmosphere before reaching the ground.^[37]

Cloud structure in the Venusian atmosphere in 1979, revealed by observations in the ultraviolet band by Pioneer Venus Orbiter

Global radar view of Venus (without the clouds) from the Magellan imaging between 1990 and 1994

Impact craters on the surface of Venus (image reconstructed from radar data)

Internal structure

Without seismic data or knowledge of its moment of inertia, little direct information is available about the internal structure and geochemistry of Venus.^[38] The similarity in size and density between Venus and Earth suggests they share a similar internal structure: a core, mantle, and crust. Like that of Earth, the Venusian core is at least partially liquid because the two planets have been cooling at about the same rate.^[39] The slightly smaller size of Venus suggests pressures are significantly lower in its deep interior than Earth. The principal difference between the two planets is the lack of evidence for plate tectonics on Venus, possibly because its crust is too strong to subduct without water to make it less viscous. This results in reduced heat loss from the planet, preventing it from cooling and providing a likely explanation for its lack of an internally generated magnetic field.^[40] Instead, Venus may lose its internal heat in periodic major resurfacing events.^[23]

Atmosphere and climate

Venus has an extremely dense atmosphere, which consists mainly of carbon dioxide and a small amount of nitrogen. The atmospheric mass is 93 times that of Earth's atmosphere, whereas the pressure at the planet's surface is about 92 times that at Earth's surface—a pressure equivalent to that at a depth of nearly 1 kilometre under Earth's oceans. The density at the surface is 65 kg/m³, 6.5% that of water. The CO₂-rich atmosphere, along with thick clouds of sulfur dioxide, generates the strongest greenhouse effect in the Solar System, creating surface temperatures of at least 735 K (462 °C).^[11][41] This makes the Venusian surface hotter than Mercury's, which has a minimum surface temperature of 55 K (−220 °C) and maximum surface temperature of 695 K (420 °C),^[42] even though Venus is nearly twice Mercury's distance from the Sun and thus receives only 25% of Mercury's solar irradiance. The surface of Venus is often described as hellish.^[43] This temperature is higher than temperatures used to achieve sterilization.
Studies have suggested that billions of years ago the Venusian atmosphere was much more like Earth's than it is now, and that there may have been substantial quantities of liquid water on the surface, but after a period of 600 million to several billion years,^[44] a runaway greenhouse effect was caused by the evaporation of that original water, which generated a critical level of greenhouse gases in its atmosphere.^[45] Although the surface conditions on the planet are no longer hospitable to any Earthlike life that may have formed before this event, it is possible that life exists in the lower and middle cloud layers of Venus.^[46][47][48]

Thermal inertia and the transfer of heat by winds in the lower atmosphere mean that the temperature of the Venusian surface does not vary significantly between the night and day sides, despite the planet's extremely slow rotation. Winds at the surface are slow, moving at a few kilometres per hour, but because of the high density of the atmosphere at the Venusian surface, they exert a significant amount of force against obstructions, and transport dust and small stones across the surface. This alone would make it difficult for a human to walk through, even if the heat, pressure and lack of oxygen were not a problem.^[49]

Above the dense CO₂ layer are thick clouds consisting mainly of sulfur dioxide and sulfuric acid droplets.^[50][51] These clouds reflect and scatter about 90% of the sunlight that falls on them back into space, and prevent visual observation of the Venusian surface. The permanent cloud cover means that although Venus is closer than Earth to the Sun, the Venusian surface is not as well lit. Strong 85 m/s (300 km/h) winds at the cloud tops circle the planet about every four to five Earth days.^[52] Venusian winds move at up to 60 times the speed of the planet's rotation, whereas Earth's fastest winds are only 10–20% rotation speed.^[53]

The surface of Venus is effectively isothermal; it retains a constant temperature not only between day and night but between the equator and the poles.^[2][54] The planet's minute axial tilt—less than 3°, compared to 23° on Earth—also minimizes seasonal temperature variation.^[55] The only appreciable variation in temperature occurs with altitude. The highest point on Venus, Maxwell Montes, is therefore the coolest point on the planet, with a temperature of about 655 K (380 °C) and an atmospheric pressure of about 4.5 MPa (45 bar).^[56][57] In 1995, the Magellan probe imaged a highly reflective substance at the tops of the highest mountain peaks that bore a strong resemblance to terrestrial snow. This substance arguably formed from a similar process to snow, albeit at a far higher temperature. Too volatile to condense on the surface, it rose in gas form to cooler higher elevations, where it then fell as precipitation. The identity of this substance is not known with certainty, but speculation has ranged from elemental tellurium to lead sulfide (galena).^[58]

The clouds of Venus are capable of producing lightning much like the clouds on Earth.^[59] The existence of lightning had been controversial since the first suspected bursts were detected by the Soviet Venera probes. In 2006–2007 Venus Express clearly detected whistler mode waves, the signatures of lightning. Their intermittent appearance indicates a pattern associated with weather activity. The lightning rate is at least half of that on Earth.^[59] In 2007 the Venus Express probe discovered that a huge double atmospheric vortex exists at the south pole.^[60][61]

Another discovery made by the Venus Express probe in 2011 is that an ozone layer exists high in the atmosphere of Venus.^[62]

On January 29, 2013, ESA scientists reported that the ionosphere of the planet Venus streams outwards in a manner similar to "the ion tail seen streaming from a comet under similar conditions."^[63][64]

Atmospheric composition

Synthetic stick absorption spectrum of a simple gas mixture corresponding to Earth's atmosphere

Venusian atmosphere composition based on HITRAN data^[65] created using Hitran on the Web system.^[66]

Green colour – water vapour, red – carbon dioxide, WN – wavenumber (other colours have different meanings, lower wavelengths on the right, higher on the left).

Magnetic field and core

In 1967, Venera 4 found the Venusian magnetic field to be much weaker than that of Earth. This magnetic field is induced by an interaction between the ionosphere and the solar wind,^[67][68] rather than by an internal dynamo in the core like the one inside Earth. Venus's small induced magnetosphere provides negligible protection to the atmosphere against cosmic radiation. This radiation may result in cloud-to-cloud lightning discharges.^[69]

The lack of an intrinsic magnetic field at Venus was surprising given it is similar to Earth in size, and was expected also to contain a dynamo at its core. A dynamo requires three things: a conducting liquid, rotation, and convection. The core is thought to be electrically conductive and, although its rotation is often thought to be too slow, simulations show it is adequate to produce a dynamo.^[70][71] This implies the dynamo is missing because of a lack of convection in the Venusian core. On Earth, convection occurs in the liquid outer layer of the core because the bottom of the liquid layer is much hotter than the top. On Venus, a global resurfacing event may have shut down plate tectonics and led to a reduced heat flux through the crust. This caused the mantle temperature to increase, thereby reducing the heat flux out of the core. As a result, no internal geodynamo is available to drive a magnetic field. Instead, the heat energy from the core is being used to reheat the crust.^[72]

One possibility is that Venus has no solid inner core,^[73] or that its core is not cooling, so that the entire liquid part of the core is at approximately the same temperature. Another possibility is that its core has already completely solidified. The state of the core is highly dependent on the concentration of sulfur, which is unknown at present.^[72]

The weak magnetosphere around Venus means that the solar wind is interacting directly with its outer atmosphere. Here, ions of hydrogen and oxygen are being created by the dissociation of neutral molecules from ultraviolet radiation. The solar wind then supplies energy that gives some of these ions sufficient velocity to escape Venus's gravity field. This erosion process results in a steady loss of low-mass hydrogen, helium, and oxygen ions, whereas higher-mass molecules, such as carbon dioxide, are more likely to be retained. Atmospheric erosion by the solar wind probably led to the loss of most of Venus's water during the first billion years after it formed. The erosion has increased the ratio of higher-mass deuterium to lower-mass hydrogen in the upper atmosphere by 150 times compared to the ratio in the lower atmosphere.^[74]

Orbit and rotation

Venus orbits the Sun at an average distance of about 108 million kilometres (about 0.7 AU) and completes an orbit every 224.65 days. Venus is the second planet from the Sun and orbits the Sun approximately 1.6 times (yellow trail) in Earth's 365 days (blue trail)

Venus orbits the Sun at an average distance of about 0.72 AU (108,000,000 km; 67,000,000 mi), and completes an orbit every 224.65 days. Although all planetary orbits are elliptical, Venus's orbit is the closest to circular, with an eccentricity of less than 0.01.^[2] When Venus lies between Earth and the Sun, a position known as inferior conjunction, it makes the closest approach to Earth of any planet at an average distance of 41 million km.^[2] The planet reaches inferior conjunction every 584 days, on average.^[2] Owing to the decreasing eccentricity of Earth's orbit, the minimum distances will become greater over tens of thousands of years. From the year 1 to 5383, there are 526 approaches less than 40 million km; then there are none for about 60,158 years.^[75]

All the planets of the Solar System orbit the Sun in an anti-clockwise direction as viewed from above Earth's north pole. Most planets also rotate on their axes in an anti-clockwise direction, but Venus rotates clockwise (called "retrograde" rotation) once every 243 Earth days—the slowest rotation period of any planet. Because its rotation is so slow, it is highly spherical.^[76] A Venusian sidereal day thus lasts longer than a Venusian year (243 versus 224.7 Earth days). Venus's equator rotates at 6.5 km/h (4.0 mph), whereas Earth's is approximately 1,670 km/h (1,040 mph).^[77] Venus's rotation has slowed down by 6.5 min per Venusian sidereal day since the Magellan spacecraft visited it 16 years ago.^[78] Because of the retrograde rotation, the length of a solar day on Venus is significantly shorter than the sidereal day, at 116.75 Earth days (making the Venusian solar day shorter than Mercury's 176 Earth days); one Venusian year is about 1.92 Venusian (solar) days long.^[79] To an observer on the surface of Venus, the Sun would rise in the west and set in the east, though the Sun cannot be seen from the surface due to Venus's opaque clouds.^[79]

Venus may have formed from the solar nebula with a different rotation period and obliquity, reaching its current state because of chaotic spin changes caused by planetary perturbations and tidal effects on its dense atmosphere, a change that would have occurred over the course of billions of years. The rotation period of Venus may represent an equilibrium state between tidal locking to the Sun's gravitation, which tends to slow rotation, and an atmospheric tide created by solar heating of the thick Venusian atmosphere.^[80][81] The 584-day average interval between successive close approaches to Earth is almost exactly equal to 5 Venusian solar days,^[82] but the hypothesis of a spin–orbit resonance with Earth has been discounted.^[83]

Venus has no natural satellites,^[84] though the asteroid 2002 VE₆₈ presently maintains a quasi-orbital relationship with it.^[85][86] Besides this quasi-satellite, it has two other temporary co-orbitals, 2001 CK32 and 2012 XE133.^[87] In the 17th century, Giovanni Cassini reported a moon orbiting Venus, which was named Neith and numerous sightings were reported over the following 200 years, but most were determined to be stars in the vicinity. Alex Alemi's and David Stevenson's 2006 study of models of the early Solar System at the California Institute of Technology shows Venus likely had at least one moon created by a huge impact event billions of years ago.^[88] About 10 million years later, according to the study, another impact reversed the planet's spin direction and caused the Venusian moon gradually to spiral inward until it collided and merged with Venus.^[89] If later impacts created moons, these were absorbed in the same way. An alternative explanation for the lack of satellites is the effect of strong solar tides, which can destabilize large satellites orbiting the inner terrestrial planets.^[84]

Observation

Venus is always brighter than the brightest stars outside the Solar System, as can be seen here over the Pacific Ocean

Phases of Venus and evolution of its apparent diameter

Venus is always brighter than any star (apart from the Sun). The greatest luminosity, apparent magnitude −4.9,^[9] occurs during crescent phase when it is near Earth. Venus fades to about magnitude −3 when it is backlit by the Sun.^[8] The planet is bright enough to be seen in a mid-day clear sky,^[90] and it can be easy to see when the Sun is low on the horizon. As an inferior planet, it always lies within about 47° of the Sun.^[10]

Venus "overtakes" Earth every 584 days as it orbits the Sun.^[2] As it does so, it changes from the "Evening Star", visible after sunset, to the "Morning Star", visible before sunrise. Although Mercury, the other inferior planet, reaches a maximum elongation of only 28° and is often difficult to discern in twilight, Venus is hard to miss when it is at its brightest. Its greater maximum elongation means it is visible in dark skies long after sunset. As the brightest point-like object in the sky, Venus is a commonly misreported "unidentified flying object". U.S. President Jimmy Carter reported having seen a UFO in 1969, which later analysis suggested was probably Venus. Countless other people have mistaken Venus for something more exotic.^[91]

As it moves around its orbit, Venus displays phases like those of the Moon in a telescopic view. The planet presents a small "full" image when it is on the opposite side of the Sun. It shows a larger "quarter phase" when it is at its maximum elongations from the Sun, and is at its brightest in the night sky, and presents a much larger "thin crescent" in telescopic views as it comes around to the near side between Earth and the Sun. Venus is at its largest and presents its "new phase" when it is between Earth and the Sun. Its atmosphere can be seen in a telescope by the halo of light refracted around it.^[10]

Transits

2004 transit of Venus

The Venusian orbit is slightly inclined relative to Earth's orbit; thus, when the planet passes between Earth and the Sun, it usually does not cross the face of the Sun. Transits of Venus occur when the planet's inferior conjunction coincides with its presence in the plane of Earth's orbit. Transits of Venus occur in cycles of 243 years with the current pattern of transits being pairs of transits separated by eight years, at intervals of about 105.5 years or 121.5 years—a pattern first discovered in 1639 by the English astronomer Jeremiah Horrocks.^[92]

The latest pair was June 8, 2004 and June 5–6, 2012. The transit could be watched live from many online outlets or observed locally with the right equipment and conditions.^[93]

The preceding pair of transits occurred in December 1874 and December 1882; the following pair will occur in December 2117 and December 2125.^[94] Historically, transits of Venus were important, because they allowed astronomers to determine the size of the astronomical unit, and hence the size of the Solar System as shown by Horrocks in 1639.^[95] Captain Cook's exploration of the east coast of Australia came after he had sailed to Tahiti in 1768 to observe a transit of Venus.^[96][97]

Ashen light

A long-standing mystery of Venus observations is the so-called ashen light—an apparent weak illumination of its dark side, seen when the planet is in the crescent phase. The first claimed observation of ashen light was made in 1643, but the existence of the illumination has never been reliably confirmed. Observers have speculated it may result from electrical activity in the Venusian atmosphere, but it could be illusory, resulting from the physiological effect of observing a bright, crescent-shaped object.^[98]

Studies

Early studies

The "black drop effect" as recorded during the 1769 transit

Venus was known to ancient civilizations both as the "morning star" and as the "evening star", names that reflect the early assumption that these were two separate objects. The Venus tablet of Ammisaduqa, dated 1581 BCE, shows the Babylonians understood the two were a single object, referred to in the tablet as the "bright queen of the sky", and could support this view with detailed observations.^[99] The Greeks thought of the two as separate stars, Phosphorus and Hesperus, until the time of Pythagoras in the sixth century BC.^[100] The Romans designated the morning aspect of Venus as Lucifer, literally "Light-Bringer", and the evening aspect as Vesper, both literal translations of the respective Greek names.

The transit of Venus was first observed in 1032 by the Persian astronomer Avicenna, who concluded Venus is closer to Earth than the Sun,^[101] and established Venus was, at least sometimes, below the Sun.^[102] In the 12th century, the Andalusian astronomer Ibn Bajjah observed "two planets as black spots on the face of the Sun", which were later identified as the transits of Venus and Mercury by the Maragha astronomer Qotb al-Din Shirazi in the 13th century.^[103] The transit of Venus was also observed by Jeremiah Horrocks on 4 December 1639 (24 November under the Julian calendar in use at that time), along with his friend, William Crabtree, at each of their respective homes.^[104]

Galileo's discovery that Venus showed phases (although remaining near the Sun in Earth's sky) proved that it orbits the Sun and not Earth

When the Italian physicist Galileo Galilei first observed the planet in the early 17th century, he found it showed phases like the Moon, varying from crescent to gibbous to full and vice versa. When Venus is furthest from the Sun in the sky, it shows a half-lit phase, and when it is closest to the Sun in the sky, it shows as a crescent or full phase. This could be possible only if Venus orbited the Sun, and this was among the first observations to clearly contradict the Ptolemaic geocentric model that the Solar System was concentric and centered on Earth.^[105][106]

The atmosphere of Venus was discovered in 1761 by Russian polymath Mikhail Lomonosov.^[107][108] Venus's atmosphere was observed in 1790 by German astronomer Johann Schröter. Schröter found when the planet was a thin crescent, the cusps extended through more than 180°. He correctly surmised this was due to scattering of sunlight in a dense atmosphere. Later, American astronomer Chester Smith Lyman observed a complete ring around the dark side of the planet when it was at inferior conjunction, providing further evidence for an atmosphere.^[109] The atmosphere complicated efforts to determine a rotation period for the planet, and observers such as Italian-born astronomer Giovanni Cassini and Schröter incorrectly estimated periods of about 24 h from the motions of markings on the planet's apparent surface.^[110]

Ground-based research

Modern telescopic view of Venus from Earth's surface

Little more was discovered about Venus until the 20th century. Its almost featureless disc gave no hint what its surface might be like, and it was only with the development of spectroscopic, radar and ultraviolet observations that more of its secrets were revealed. The first UV observations were carried out in the 1920s, when Frank E. Ross found that UV photographs revealed considerable detail that was absent in visible and infrared radiation. He suggested this was due to a dense, yellow lower atmosphere with high cirrus clouds above it.^[111]

Spectroscopic observations in the 1900s gave the first clues about the Venusian rotation. Vesto Slipher tried to measure the Doppler shift of light from Venus, but found he could not detect any rotation. He surmised the planet must have a much longer rotation period than had previously been thought.^[112] Later work in the 1950s showed the rotation was retrograde. Radar observations of Venus were first carried out in the 1960s, and provided the first measurements of the rotation period, which were close to the modern value.^[113]

Radar observations in the 1970s revealed details of the Venusian surface for the first time. Pulses of radio waves were beamed at the planet using the 300 m (980 ft) radio telescope at Arecibo Observatory, and the echoes revealed two highly reflective regions, designated the Alpha and Beta regions. The observations also revealed a bright region attributed to mountains, which was called Maxwell Montes.^[114] These three features are now the only ones on Venus that do not have female names.^[115]

Exploration

Early efforts

Mariner 2, launched in 1962

The first robotic space probe mission to Venus, and the first to any planet, began on 12 February 1961, with the launch of the Venera 1 probe. The first craft of the otherwise highly successful Soviet Venera program, Venera 1 was launched on a direct impact trajectory, but contact was lost seven days into the mission, when the probe was about 2 million km from Earth. It was estimated to have passed within 100,000 km of Venus in mid-May.^[116]

The United States exploration of Venus also started badly with the loss of the Mariner 1 probe on launch. The subsequent Mariner 2 mission, after a 109-day transfer orbit on 14 December 1962, became the world's first successful interplanetary mission, passing 34,833 km above the surface of Venus. Its microwave and infrared radiometers revealed that although the Venusian cloud tops were cool, the surface was extremely hot—at least 425 °C, confirming previous Earth-based measurements^[117] and finally ending any hopes that the planet might harbour ground-based life. Mariner 2 also obtained improved estimates of its mass and of the astronomical unit, but was unable to detect either a magnetic field or radiation belts.^[118]

Atmospheric entry

Pioneer Venus Multiprobe

The Soviet Venera 3 probe crash-landed on Venus on 1 March 1966. It was the first man-made object to enter the atmosphere and strike the surface of another planet. Its communication system failed before it was able to return any planetary data.^[119] On 18 October 1967, Venera 4 successfully entered the atmosphere and deployed science experiments. Venera 4 showed the surface temperature was even hotter than Mariner 2 had measured, at almost 500 °C, and the atmosphere was 90 to 95% carbon dioxide. The Venusian atmosphere was considerably denser than Venera 4's designers had anticipated, and its slower than intended parachute descent meant its batteries ran down before the probe reached the surface. After returning descent data for 93 minutes, Venera 4's last pressure reading was 18 bar at an altitude of 24.96 km.^[119]

One day later on 19 October 1967, Mariner 5 conducted a fly-by at a distance of less than 4000 km above the cloud tops. Mariner 5 was originally built as a backup for the Mars-bound Mariner 4; when that mission was successful, the probe was refitted for a Venus mission. A suite of instruments more sensitive than those on Mariner 2, in particular its radio occultation experiment, returned data on the composition, pressure and density of the Venusian atmosphere.^[120] The joint Venera 4 – Mariner 5 data was analysed by a combined Soviet-American science team in a series of colloquia over the following year,^[121] in an early example of space cooperation.^[122]

Armed with the lessons and data learned from Venera 4, the Soviet Union launched the twin probes Venera 5 and Venera 6 five days apart in January 1969; they encountered Venus a day apart on 16 and 17 May. The probes were strengthened to improve their crush depth to 25 bar and were equipped with smaller parachutes to achieve a faster descent. Because then-current atmospheric models of Venus suggested a surface pressure of between 75 and 100 bar, neither was expected to survive to the surface. After returning atmospheric data for a little over 50 minutes, they were both crushed at altitudes of approximately 20 km before going on to strike the surface on the night side of Venus.^[119]

Surface and atmospheric science

Venera 7 represented an effort to return data from the planet's surface, and was constructed with a reinforced descent module capable of withstanding a pressure of 180 bar. The module was precooled before entry and equipped with a specially reefed parachute for a rapid 35-minute descent. While entering the atmosphere on 15 December 1970, the parachute is believed to have partially torn, and the probe struck the surface with a hard, yet not fatal, impact. Probably tilted onto its side, it returned a weak signal, supplying temperature data for 23 minutes, the first telemetry received from the surface of another planet.^[119]

180-degree panorama of the Venusian surface from the Soviet Venera 9 lander

The Venera program continued with Venera 8 sending data from the surface for 50 minutes, after entering the atmosphere on 22 July 1972. Venera 9, which entered the atmosphere of Venus on 22 October 1975, and Venera 10, which entered the atmosphere three days later, sent the first images of the Venusian landscape. The two landing sites presented different terrains in the immediate vicinities of the landers: Venera 9 had landed on a 20-degree slope scattered with boulders around 30–40 cm across; Venera 10 showed basalt-like rock slabs interspersed with weathered material.^[123]

The Pioneer Venus orbiter

In the meantime, the United States had sent the Mariner 10 probe on a gravitational slingshot trajectory past Venus on its way to Mercury. On 5 February 1974, Mariner 10 passed within 5790 km of Venus, returning over 4000 photographs as it did so. The images, the best then achieved, showed the planet to be almost featureless in visible light, but ultraviolet light revealed details in the clouds that had never been seen in Earth-bound observations.^[124]

The American Pioneer Venus project consisted of two separate missions.^[125] The Pioneer Venus Orbiter was inserted into an elliptical orbit around Venus on 4 December 1978, and remained there for over 13 years, studying the atmosphere and mapping the surface with radar. The Pioneer Venus Multiprobe released a total of four probes, which entered the atmosphere on 9 December 1978, returning data on its composition, winds and heat fluxes.^[126]

Position of Venera landing sites returning images form the surface

Four more Venera lander missions took place over the next four years, with Venera 11 and Venera 12 detecting Venusian electrical storms;^[127] and Venera 13 and Venera 14, landing on 1 and 5 March 1982, returning the first colour photographs of the surface. All four missions deployed parachutes for braking in the upper atmosphere, then released them at altitudes of 50 km, the dense lower atmosphere providing enough friction to allow for unaided soft landings. Both Venera 13 and 14 analysed soil samples with an on-board X-ray fluorescence spectrometer, and attempted to measure the compressibility of the soil with an impact probe.^[127] Venera 14 struck its own ejected camera lens cap and its probe failed to contact the soil.^[127] The Venera program came to a close in October 1983, when Venera 15 and Venera 16 were placed in orbit to conduct mapping of the Venusian terrain with synthetic aperture radar.^[128]

In 1985, the Soviet Union took advantage of the opportunity to combine missions to Venus and Comet Halley, which passed through the inner Solar System that year. En route to Halley, on 11 and 15 June 1985, the two spacecraft of the Vega program each dropped a Venera-style probe (of which Vega 1's partially failed) and released a balloon-supported aerobot into the upper atmosphere. The balloons achieved an equilibrium altitude of around 53 km, where pressure and temperature are comparable to those at Earth's surface. They remained operational for around 46 hours, and discovered the Venusian atmosphere was more turbulent than previously believed, and subject to high winds and powerful convection cells.^[129][130]

Radar mapping

Magellan radar topographical map of Venus (false colour)

Early Earth-based radar provided a basic idea of the surface. The Pioneer Venus and the Veneras provided improved resolution.

The United States' Magellan probe was launched on 4 May 1989, with a mission to map the surface of Venus with radar.^[27] The high-resolution images it obtained during its 4½ years of operation far surpassed all prior maps and were comparable to visible-light photographs of other planets. Magellan imaged over 98% of the Venusian surface by radar,^[131] and mapped 95% of its gravity field. In 1994, at the end of its mission, Magellan was sent to its destruction into the atmosphere of Venus to quantify its density.^[132] Venus was observed by the Galileo and Cassini spacecraft during fly-bys on their respective missions to the outer planets, but Magellan was the last dedicated mission to Venus for over a decade.^[133][134]

Current and future missions

NASA's MESSENGER mission to Mercury performed two fly-bys of Venus in October 2006 and June 2007, to slow its trajectory for an eventual orbital insertion of Mercury in March 2011. It collected scientific data on Venus during both fly-bys.^[135]

The Venus Express probe was designed and built by the European Space Agency. Launched on 9 November 2005 by a Russian Soyuz-Fregat rocket procured through Starsem, it successfully assumed a polar orbit around Venus on 11 April 2006.^[136] The probe is undertaking a detailed study of the Venusian atmosphere and clouds, including mapping of the planet's plasma environment and surface characteristics, particularly temperatures. One of the first results from Venus Express is the discovery that a huge double atmospheric vortex exists at the southern pole.^[136]

Artist's impression of a Stirling cooled Venus Rover.^[137]

The Japan Aerospace Exploration Agency (JAXA) devised a Venus orbiter, Akatsuki (formerly "Planet-C"), which was launched on 20 May 2010, but the craft failed to enter orbit in December 2010. Hopes remain that the probe can successfully hibernate and make another insertion attempt in six years. Planned investigations included surface imaging with an infrared camera and experiments designed to confirm the presence of lightning, as well as the determination of the existence of current surface volcanism.^[138]

The European Space Agency (ESA) hopes to launch a mission to Mercury in 2016, called BepiColombo, which will perform two fly-bys of Venus before it reaches Mercury orbit in 2020.^[139][140]

NASA will launch the Solar Probe Plus in 2018, which will perform seven Venus fly-bys during its six year, 24 orbit reconscience of the Sun.^[141]

Under its New Frontiers Program, NASA has proposed a lander mission called the Venus In-Situ Explorer to land on Venus to study surface conditions and investigate the elemental and mineralogical features of the regolith. The probe would be equipped with a core sampler to drill into the surface and study pristine rock samples not weathered by the harsh surface conditions. A Venus atmospheric and surface probe mission, "Surface and Atmosphere Geochemical Explorer" (SAGE), was selected by NASA as a candidate mission study in the 2009 New Frontiers selection,^[142] but the mission was not selected for flight.

Venus aircraft concept

The Venera-D (Russian: Венера-Д) probe is a proposed Russian space probe to Venus, to be launched around 2016, to make remote-sensing observations around the planet and deploying a lander, based on the Venera design, capable of surviving for a long duration on the surface. Other proposed Venus exploration concepts include rovers, balloons, and aeroplanes.^[143]

In late 2013 the Venus Spectral Rocket Experiment took place, which launched a sub-orbital space telescope.

Manned fly-by concept

A manned Venus fly-by mission, using Apollo program hardware, was proposed in the late 1960s.^[144] The mission was planned to launch in late October or early November 1973, and would have used a Saturn V to send three men to fly past Venus in a flight lasting approximately one year. The spacecraft would have passed approximately 5,000 km (3,100 mi) from the surface of Venus about four months later.^[144] Inspiration Mars includes a manned Venus flyby in their 2021 mission.^[145]

Sample return

Various concepts for a Venus sample return include a high-speed upper atmosphere collection, an atmosphere sample return by slowing down and entering then returning, and a surface sample return.^[146]

Spacecraft timeline

This is a list of attempted and successful spacecraft that have left Earth to explore Venus more closely.^[147] Venus has also been imaged by the Hubble Space Telescope in Earth orbit, and distant telescopic observations are another source of information about Venus.

Timeline by NASA Goddard Space Flight Center (up to 2011)^[147]

Responsible	Mission	Launch	Elements and result	Notes
USSR	Sputnik 7	01961-02-04-00004 February 1961	Impact (attempted)
USSR	Venera 1	01961-02-12-000012 February 1961	Fly-by (contact lost)
USA	Mariner 1	01962-07-22-000022 July 1962	Fly-by (launch failure)
USSR	Sputnik 19	01962-08-25-000025 August 1962	Fly-by (attempted)
USA	Mariner 2	01962-08-27-000027 August 1962	Fly-by	First successful planetary flyby[148]
USSR	Sputnik 20	01962-09-01-00001 September 1962	Fly-by (attempted)
USSR	Sputnik 21	01962-09-12-000012 September 1962	Fly-by (attempted)
USSR	Cosmos 21	01963-11-11-000011 November 1963		Attempted Venera test flight?
USSR	Venera 1964A	01964-02-19-000019 February 1964	Fly-by (launch failure)
USSR	Venera 1964B	01964-03-01-00001 March 1964	Fly-by (launch failure)
USSR	Cosmos 27	01964-03-27-000027 March 1964	Fly-by (attempted)
USSR	Zond 1	01964-04-02-00002 April 1964	Fly-by (contact lost)
USSR	Venera 2	01965-11-12-000012 November 1965	Fly-by (contact lost)
USSR	Venera 3	01965-11-16-000016 November 1965	Lander (contact lost)
USSR	Cosmos 96	01965-11-23-000023 November 1965	Lander (attempted?)
USSR	Venera 1965A	01965-11-23-000023 November 1965	Fly-by (launch failure)
USSR	Venera 4	01967-06-12-000012 June 1967	Probe
USA	Mariner 5	01967-06-14-000014 June 1967	Fly-by
USSR	Cosmos 167	01967-06-17-000017 June 1967	Probe (attempted)
USSR	Venera 5	01969-01-05-00005 January 1969	Probe
USSR	Venera 6	01969-01-10-000010 January 1969	Probe
USSR	Venera 7	01970-08-17-000017 August 1970	Lander
USSR	Cosmos 359	01970-08-22-000022 August 1970	Probe (attempted)
USSR	Venera 8	01972-03-27-000027 March 1972	Probe
USSR	Cosmos 482	01972-03-31-000031 March 1972	Probe (attempted)
USA	Mariner 10	01973-11-04-00004 November 1973	Fly-by	Mercury fly-by
USSR	Venera 9	01975-06-08-00008 June 1975	Orbiter and lander
USSR	Venera 10	01975-06-14-000014 June 1975	Orbiter and lander
USA	Pioneer Venus 1	01978-05-20-000020 May 1978	Orbiter
USA	Pioneer Venus 2	01978-08-08-00008 August 1978	Probes
USSR	Venera 11	01978-09-09-00009 September 1978	Fly-by bus and lander
USSR	Venera 12	01978-09-14-000014 September 1978	Fly-by bus and lander
USSR	Venera 13	01981-10-30-000030 October 1981	Fly-by bus and lander
USSR	Venera 14	01981-11-04-00004 November 1981	Fly-by bus and lander
USSR	Venera 15	01983-06-02-00002 June 1983	Orbiter
USSR	Venera 16	01983-06-07-00007 June 1983	Orbiter
USSR	Vega 1	01984-12-15-000015 December 1984	Lander and balloon	Comet Halley fly-by
USSR	Vega 2	01984-12-21-000021 December 1984	Lander and balloon	Comet Halley fly-by
USA	Magellan	01989-05-04-00004 May 1989	Orbiter
USA	Galileo	01989-10-18-000018 October 1989	Fly-by	Jupiter orbiter/probe
USA	Cassini	01997-10-15-000015 October 1997	Fly-by	Saturn orbiter
USA	MESSENGER	02004-08-03-00003 August 2004	Flyby (x2)	Mercury orbiter
ESA	Venus Express	02005-11-09-00009 November 2005	Orbiter
JPN	Akatsuki	02010-12-07-00007 December 2010	Orbiter (attempted)	Possible reattempt in 2016 or 2018
ESA JPN	BepiColombo		Two flybys planned	Planned Mercury orbiter

Venera-D is a possible Russian mission in the 2020s^[149]

In culture

Throughout history and cultures, the planet has been of remarkable importance as an especial object of observation, reflection and projection. Popular beliefs and observations resulted in different and in parts similar patterns in mythology as well as phenomenological descriptions, attributions and depictions, e.g. in astrology. Such developments in manifestations of human thought reflect the planet's image as a result of early observations of Venus and their impact on culture and science.

Etymology

The adjective Venusian is commonly used for items related to Venus, though the Latin adjective is the rarely used Venerean; the archaic Cytherean is still occasionally encountered. Venus is the only planet in the Solar System that is named after a female figure.^[a] (Three dwarf planets – Ceres, Eris and Haumea – along with many of the first discovered asteroids^[150] and some moons (such as the Galilean moons) also have feminine names. Earth and the Moon also have feminine names in many languages—Gaia/Terra, Selene/Luna—but the female mythological figures who personified them were named after them, not the other way around.)^[151]

Venus symbol

The astronomical symbol for Venus is the same as that used in biology for the female sex: a circle with a small cross beneath.^[152] The Venus symbol also represents femininity, and in Western alchemy stood for the metal copper.^[152] Polished copper has been used for mirrors from antiquity, and the symbol for Venus has sometimes been understood to stand for the mirror of the goddess.^[152]

Colonization and terraforming

Artist's conception of a terraformed Venus

Owing to its extremely hostile conditions, a surface colony on Venus is not possible with current technology. The atmospheric pressure and temperature approximately fifty kilometres above the surface are similar to those at Earth's surface and Earth air (nitrogen and oxygen) would be a lifting gas in the Venusian atmosphere of mostly carbon dioxide. This has led to proposals for "floating cities" in the Venusian atmosphere.^[153] Aerostats (lighter-than-air balloons) could be used for initial exploration and ultimately for permanent settlements.^[153] Among the many engineering challenges are the dangerous amounts of sulfuric acid at these heights.^[153]

Giant Asteroid Collision May Have Radically Transformed Mars

An ancient, global-scale impact could explain the Red Planet’s mysterious “two-faced” appearance

February 25, 2015 |By Robin Wylie

 

Original link:  http://www.scientificamerican.com/article/giant-asteroid-collision-may-have-radically-transformed-mars/?WT.mc_id=SA_Facebook 

When the team simulated a collision with an asteroid about 4,000 kilometers across (slightly larger than Earth’s moon) they found that it caused the crust of the “virtual” Mars to reform into two distinct zones.
Credit: USGS

The planet Mars has been associated with its namesake god of war for millennia, but its own past may have been more violent than was previously imagined. A new study suggests that Mars was once hit by an asteroid so large that it melted nearly half of the planet’s surface.

Researchers came to this conclusion while studying a strange feature known as the Martian hemispheric dichotomy—a dramatic drop in surface elevation and crustal thickness that occurs near Mars’ equator. In the northern hemisphere the land’s elevation is on average about 5.5 kilometers lower and the crust is around 26 kilometers thinner.

The dichotomy was discovered in the early 1970s when NASA’s Mariner 9 probe made the first detailed map of the Martian surface. The feature has perplexed astronomers ever since. Previous studies hinted that the dichotomy was formed by a glancing asteroid strike near the Martian north pole. But the new work, published in Geophysical Research Letters in December, suggests that a far more violent impact, at the opposite end of the planet, may have been the actual cause.

In the study astronomers at the Swiss Federal Institute of Technology (E.T.H. Zurich) used an advanced 3-D computer model to simulate the effect of an asteroid impact on Mars 4.5 billion years ago, when experts think the dichotomy formed. They tested a rival hypothesis for its origin—that it had been formed by an impact at Mars’s south pole.

When the team simulated a collision with an asteroid about 4,000 kilometers across (slightly larger than Earth’s moon) they found that it caused the crust of the “virtual” Mars to reform into two distinct zones: a thicker one in the southern hemisphere and a thinner one in the north, similar to what we see on the real planet. What’s more, the predicted thicknesses of the two crustal segments matched the real values observed on Mars almost exactly. Taken together these predictions provide compelling evidence that a south polar impact was the cause of the dichotomy. “This study advances an alternate impact origin for the Martian dichotomy,” says Craig Agnor, an astronomer at Queen Mary, University of London, who was not involved in the work.

The simulation predicted that the impact would have generated so much heat that large swathes of Mars’s crust would have melted, forming a “magma ocean” across most of the planet’s southern hemisphere. It also predicted that, as the molten rock subsequently cooled and solidified, it would leave a thicker, higher-elevation crust over part of that hemisphere.

These findings do not conclusively solve the mystery of the dichotomy's origin. The Swiss team’s model is not perfect; for example, it cannot explain the dichotomy’s exact size. And in any case, it is not possible to prove a hypothesis using only a computer model. But there is another reason to think that the southern impact hypothesis might be right: It sheds light on another oddity of Mars's surface—the locations of its volcanoes.

When large asteroids hit rocky planets they tend to induce volcanic activity by causing “plumes” of hot rock to rise up within the planet's mantle, many years later. A drawback of the previous, “northern” impact scenario was that the high northern latitudes of Mars contain relatively few volcanoes, which occur mostly in equatorial and southern latitudes. But the southern impact simulation predicted that a few million years after the asteroid struck, volcanic plumes would slowly begin to rise toward the surface, at first near the equator and then gradually migrating toward the south pole. This prediction agrees well with the actual locations of the Red Planet’s volcanoes.

Asteroid impacts of the scope suggested by this study are extremely unlikely to happen today. They were probably more common in the early days of the solar system, when it was still littered with the rocky debris left over from planet-building. But even then such events would have been extremely uncommon. “This result has the potential to significantly change our understanding of Mars’s past,” says Giovanni Leone, a planetary scientist at E.T.H. Zurich and the study's lead author. “A rare event may have occurred early in its history that shaped the planet as we see it today.”

Mutiny on the Bounty

From Wikipedia, the free encyclopedia

The mutineers turning Bligh and some of the officers and crew adrift from His Majesty's Ship Bounty, 29 April 1789. By Robert Dodd.

The Mutiny on the Bounty was a mutiny aboard the Royal Navy ship HMS Bounty on 28 April 1789. The mutiny was led by Fletcher Christian against their captain, Lieutenant William Bligh. According to accounts, the sailors were attracted to the "idyllic" life and sexual opportunities afforded on the Pacific island of Tahiti. It has also been argued that they were motivated by Bligh's allegedly harsh treatment of them.

Eighteen mutineers set Bligh afloat in a small boat with eighteen of the twenty-two crew loyal to him. To avoid detection and prevent desertion, the mutineers then variously settled on Pitcairn Island or on Tahiti and burned Bounty off Pitcairn.

In an extraordinary feat of seamanship, Bligh navigated the 23-foot (7 m) open launch on a 47-day voyage to Timor in the Dutch East Indies, equipped with a quadrant and pocket watch and without charts or compass. He recorded the distance as 3,618 nautical miles (6,701 km; 4,164 mi). He then returned to Britain and reported the mutiny to the Admiralty on 15 March 1790, 2 years and 11 weeks after his original departure.

The British government dispatched HMS Pandora to capture the mutineers, and Pandora reached Tahiti on 23 March 1791. Four of the men from Bounty came on board soon after her arrival, and ten more were arrested within a few weeks. These fourteen were imprisoned in a makeshift cell on Pandora's deck. Pandora ran aground on part of the Great Barrier Reef on 29 August 1791, with the loss of 31 of the crew and four of the prisoners. The surviving ten prisoners were eventually repatriated to England, tried in a naval court, with three hanged, four acquitted, and three pardoned.

Descendants of some of the mutineers and Tahitians still live on Pitcairn. The mutiny has been commemorated in books, films, and songs.

Bounty and her 1787 expedition

The ship and mission

His Majesty's Ship (HMS) Bounty began her career as the collier Bethia, a small vessel built in 1784 at the Blaydes shipyard in Hull. On 26 May 1787 (JJ Colledge/D Lyon say 23 May), she was bought by the Royal Navy for £2,600, refitted and renamed Bounty.^[1] Bligh was appointed commanding lieutenant of Bounty on 16 August 1787, at the age of 32, after a career that included a tour as sailing master of James Cook's HMS Resolution during Cook's third and final voyage (1776–79).
The Royal Navy bought the ship for a single mission in support of an experiment: she was to travel to Tahiti; pick up breadfruit plants; and transport them to the West Indies, in the hope that they would grow well there and become a cheap source of food for slaves. The experiment, promoted through a prize offered by the Royal Society, was proposed by Sir Joseph Banks, who recommended Bligh as commander, Banks at the time being the unofficial director of Kew Gardens.

In June 1787, Bounty was refitted at Deptford. The captain's great cabin was converted to house the potted breadfruit plants, and glazed windows were fitted to the upper deck, while a lead lining was installed on the floor to catch and re-use run-off water used to feed the plants. Bligh was quartered in a small cramped cabin next to crew and officers.^[2]

Outward voyage and arrival

Bligh transplanting breadfruit trees from Tahiti

On 23 December 1787, Bounty sailed from Spithead for Tahiti with a complement of 46 officers and men. For a full month, she attempted to round Cape Horn, but adverse weather blocked her. Bligh ordered her turned about, and proceeded east, rounding the Cape of Good Hope and crossing the width of the Indian Ocean. During the outward voyage, Bligh demoted the ship's sailing master, John Fryer, replacing him with Fletcher Christian. This act seriously damaged the relationship between Bligh and Fryer, and Fryer would later claim Bligh's act was entirely personal. Bounty reached Tahiti on 26 October 1788, after ten months at sea.

Bligh and his crew spent five months in Tahiti, then known as "Otaheite," collecting and preparing a total of 1,015 breadfruit plants; the five-month layover was unplanned, required to allow the plants to reach the point of development where they could be safely transported by ship. Bligh allowed the crew to live ashore and care for the potted breadfruit plants, and they became socialized to the customs and culture of the Tahitians. Many of the seamen and some of the "young gentlemen" had themselves tattooed in native fashion. Master's Mate and Acting Lieutenant Fletcher Christian married Maimiti, a Tahitian woman. Other warrant officers and seamen of the Bounty were also said to have formed "connections" with native women.

Bligh was not surprised by his crew's reaction to the Tahitians. He recorded his analysis:

The women are handsome ... and have sufficient delicacy to make them admired and beloved – The chiefs have taken such a liking to our people that they have rather encouraged their stay among them than otherwise, and even made promises of large possessions. Under these and many other attendant circumstances equally desirable it is therefore now not to be wondered at ... that a set of sailors led by officers and void of connections ... should be governed by such powerful inducement ... to fix themselves in the midst of plenty in the finest island in the world where they need not labour, and where the allurements of dissipation are more than equal to anything that can be conceived.

— A Narrative of the Mutiny, etc., by Lieut. W. Bligh, 1790, p. 9.

Tensions rise

Despite the relaxed atmosphere, relations between Bligh and his men, and particularly between Bligh and Christian, continued to deteriorate. Christian was routinely humiliated by the captain—often in front of the crew and the native Tahitians—for real or imagined slackness,^[3] while severe punishments were handed out to men whose carelessness had led to the loss or theft of equipment.^[4]
Floggings, rarely administered during the outward voyage, now became a common occurrence; as a consequence, crewmen Millward, Muspratt, and Churchill deserted the ship. They were quickly recaptured, and a search of their belongings revealed a list of names which included those of Christian and Heywood. Bligh confronted the pair and accused them of complicity in the desertion plot, which they strenuously denied; without further corroboration, Bligh could not act against them.^[3]

As the date for departure grew closer, Bligh's outbursts against his officers became more frequent.^[5] One witness reported: "Whatever fault was found, Mr. Christian was sure to bear the brunt."^[6] Tensions rose among the men, who faced the prospect of a long and dangerous voyage that would take them through the uncharted Endeavour Strait, followed by many months of hard sailing. Bligh was impatient to be away, but in Hough's words he "failed to anticipate how his company would react to the severity and austerity of life at sea ... after five dissolute, hedonistic months at Tahiti".^[7] On 5 April, Bounty finally weighed anchor and made for the open sea with her breadfruit cargo.^[5]

The mutiny

The mutiny occurred on 28 April 1789, some 23 days out and 1,300 miles west of Tahiti. Fletcher Christian had that morning contemplated making a raft and deserting the ship by paddling around 30 nautical miles (56 km; 35 mi) to the nearby island of Tofua.^[8] Instead he and several of his followers entered Bligh's cabin, which he always left unlocked. Bligh was awakened and, wearing only his nightshirt, pushed on deck where he was guarded by Christian holding a bayonet. When Bligh entreated Christian to be reasonable, Christian would only reply: "I am in hell, I am in hell!" Despite strong words and threats on both sides, the ship was taken bloodlessly and apparently without struggle by any of the loyalists except Bligh himself. Of the 42 men on board aside from Bligh and Christian, 18 joined the mutiny, two were passive, and 22 remained loyal to Bligh.

The mutineers ordered Bligh, the ship's master, two midshipmen, the surgeon's mate (Ledward), and the ship's clerk into Bounty's launch. Several more men voluntarily joined Bligh rather than remaining aboard, as they knew that those who remained on board would be considered de jure mutineers under the Articles of War.

Bligh's epic voyage

William Bligh in 1814, many years after the events described here.

In all, eighteen of the loyal crew were in the launch with Bligh; four other loyalists were forced to stay with the eighteen mutineers and two passive crew. Bligh and his crew headed for Tofua (in a bay that they subsequently called "Murderers' Cove") to augment their meager provisions.^[9] The only casualty during this voyage was a crewman, John Norton, who was stoned to death by some natives of Tofua.

Bligh then navigated the 23-foot (7 m) open launch on a 47-day voyage to Timor in the Dutch East Indies. Equipped with a quadrant and a pocket watch and with no charts or compass, he recorded the distance as 3,618 nautical miles (6,701 km; 4,164 mi). He was chased by cannibals in what is now known as Bligh Water, Fiji, and passed through the Torres Strait along the way, landing in Kupang, Timor, on 14 June.^[10] Shortly after the launch reached Timor, the cook and botanist died. Three other crewmen died in the coming months.

Lieutenant Bligh returned to Britain and reported the mutiny to the Admiralty on 15 March 1790, 2 years and 11 weeks after leaving England.

Mutineers in Tahiti

Meanwhile, the mutineers sailed for the island of Tubuai, where they tried to settle. After three months of being attacked by the island's natives they returned to Tahiti. Twelve of the mutineers and the four loyalists who had been unable to accompany Bligh remained there, taking their chances that the Royal Navy would not find them and bring them to justice.

Two of the mutineers died in Tahiti between 1789 and 1790. Matthew Thompson shot Charles Churchill and was subsequently stoned to death by Churchill's Tahitian family in an act of vendetta.

Last voyage of Pandora

HMS Pandora in the act of foundering
by Robert Batty

HMS Pandora, under the command of Captain Edward Edwards, was dispatched on 7 November 1790 to search for Bounty and the mutineers. Pandora carried twice the normal complement of master's mates, petty officers, and midshipmen, as it was expected that the extras would man Bounty when she was recovered from the mutineers.

Pandora reached Tahiti on 23 March 1791. Four of the men from Bounty came on board Pandora soon after her arrival, and ten more were arrested within a few weeks. These fourteen, mutineers and loyal crew alike, were imprisoned in a makeshift cell on Pandora's deck, which they derisively called "Pandora's Box".

On 8 May 1791, Pandora left Tahiti, spending about three months visiting islands to the west of Tahiti in search of Bounty and the remaining mutineers, without finding anything except flotsam (including some spars and a yard on Palmerston Island). Heading west through the Torres Strait, Pandora ran aground on a reef (part of the Great Barrier Reef) on 29 August 1791. The ship sank the next morning, and 31 of the crew and four of the prisoners (Skinner, Sumner, Stewart, and Hillbrandt) were lost. The remaining 89 of the ship's company and ten prisoners (released from their cell at the last moment by William Moulter, a boatswain's mate on the Pandora^[11]) assembled in four small launches, and sailed for Timor, in a voyage similar to that of Bligh. They arrived at Timor on 16 September 1791.

Court-martial

Peter Heywood, Captain Royal Navy.

After being repatriated to Britain, the ten surviving prisoners were tried by a naval court. During the trial, great importance was attached to which men had been seen to be holding weapons during the critical moments of the mutiny, as under the Articles of War, failure to act when able to prevent a mutiny was considered no different from being an active mutineer. In the judgement delivered on 18 September 1792, four men whom Bligh had designated as innocent were acquitted. Two were found guilty, but pardoned; one of these was Peter Heywood, who later rose to the rank of captain himself; the second was James Morrison, who also continued his naval career and died at sea. Another was reprieved due to a legal technicality and later also received a pardon. The other three men were convicted, and hanged aboard HMS Brunswick on 29 October 1792. In other trials, both Bligh and Edwards were court-martialled for the loss of their ships (an automatic proceeding under British naval law, and not indicative of any particular suspicion of guilt). Both were acquitted.

Bligh resumed his naval career and went on to attain the rank of Vice Admiral. His career was marked by another insurrection. In 1808, while Bligh was Governor of New South Wales, troops of New South Wales arrested him in an incident known as the Rum Rebellion.

Second breadfruit expedition

Even before Edwards had returned from his search for Bounty, HMS Providence and her tender Assistant began a second voyage to collect breadfruit trees on 3 August 1791. This mission was again championed by Joseph Banks and again commanded by Bligh, now promoted from Lieutenant to Captain. On this second voyage, they collected 2,126 breadfruit plants and hundreds of other botanical specimens. Departing Tahiti on 19 July 1792, Bligh once again successfully navigated the Torres Strait, and delivered the breadfruit to the West Indies. The slaves on Jamaica, however, refused to eat the breadfruit, so the main purpose of the expedition was initially a failure. However, breadfruit is today a staple in Jamaica.

Mutineers on Pitcairn Island

Map showing Bounty's movements in the Pacific Ocean, 1788–1790

  Voyage of Bounty to Tahiti and to location of the mutiny, 28 April 1789

  Movements of Bounty after the mutiny, under Christian's command

  Course of Bligh's open-boat journey to Coupang

Rudder in the Fiji Museum

Immediately after setting sixteen men ashore in Tahiti in September 1789,^[12] Fletcher Christian, eight other crewmen,^[13] six Tahitian men, and 18 women, one with a baby,^[14] set sail in the Bounty hoping to elude the Royal Navy. According to a journal kept by Edward Young, one of the mutineers, all but three of the Tahitian "women brought to Pitcairn had been kidnapped"^[14] when Christian set sail without warning them, the purpose being to kidnap the women.

The mutineers passed through the Fiji and Cook Islands, but feared that they would be found there. Continuing their quest for a safe haven, on 15 January 1790, they rediscovered Pitcairn Island, which had been misplaced on the Royal Navy's charts. After the decision was made to settle on Pitcairn, livestock and other provisions were removed from Bounty. To prevent the ship's detection, and anyone's possible escape, the ship was burned on 23 January 1790 in what is now called Bounty Bay. Some of her remains, such as her ballast stones, are still partially visible in its waters. Her rudder is displayed in the Fiji Museum in Suva. An anchor of Bounty was recovered by Luis Marden in Bounty Bay in 1957.

The Pitcairn Island community began life with bright prospects. There was ample food, water, and land for everyone, and the climate was mild. Although many of the Polynesians were homesick, and the Britons knew they were marooned on Pitcairn forever, they settled into life on Pitcairn fairly quickly. A number of children were born.

At the time the community on Pitcairn was first visited by outsiders, John Adams "was the sole surviving mutineer".^[15] Little is agreed upon regarding Fletcher Christian's role once the mutineers were established on Pitcairn Island. Adams claimed "Christian 'was always cheerful'" but also claimed Christian would: "retreat and brood [in a cave, and] had 'by many acts of cruelty and inhumanity, brought on himself the hatred and detestation of his companions.'"^[16] Adams variously claimed that Christian had been killed "in a single massacre that occurred on the island about four years after arrival" and that Christian had "committed suicide".^[16] Adams at another point claimed the "mutineers had divided into parties, 'seeking every opportunity on both sides to put each other to death.'"^[17] While the details were inconsistent, Adams usually agreed with the journal of Young: that Christian died as the result of a massacre: "The massacre ... had taken place in several waves of violence, and principally arose from the fact that the Englishmen had come to regard their [Tahitian] friends as slaves."^[18] The women, "passed around from one 'husband' to the other, as men died and the balance of power shifted", eventually "rebelled" as well.^[19]

Death of Fletcher Christian

In 1793, a conflict broke out on Pitcairn Island between the mutineers and the Tahitian men who sailed with them. Fletcher Christian and four of the mutineers (Jack Williams, Isaac Martin, John Mills, and William Brown) were killed by the Tahitians. All six of the Tahitian men were killed during the on-and-off fighting, some by the widows of the murdered mutineers and others by each other.

Fletcher Christian was survived by Maimiti and their son Thursday October Christian (sometimes called "Friday October Christian"). Rumours persisted that Christian left the island and made it back to England. There are other reports that Christian actually committed suicide.

Christian's death caused a leadership vacuum on the island. Two of the four surviving mutineers, Ned Young and John Adams (also known as Alexander Smith), assumed leadership, and some peace followed, until William McCoy created a still and began brewing an alcoholic beverage from a native plant. The mutineers began drinking excessively and making life miserable for the women.

The women revolted a number of times—with the men continually "granting pardons" (each time threatening to execute the leaders of the next revolt)—and some of the women attempted to leave the island on a makeshift raft; it swamped in the "bay". Life in Pitcairn continued thus until the deaths of McCoy and Quintal, and the destruction of the still.

William McCoy died after a drunken fall. Matthew Quintal was subsequently killed by John Adams and Ned Young after threatening to kill everyone. Eventually John Adams and Ned Young were reconciled with the women, and the community began to flourish.

Ned Young succumbed in 1800 to asthma, the first man to die of natural causes. After Young's death in 1800, Adams became the leader of the community, and took responsibility for educating its members. Adams started holding regular Sunday services and teaching the Christian religion to the settlement. His gentleness and tolerance enabled the small community to thrive, and peace was restored to Pitcairn Island, with the population measuring one man, nine Tahitian women and dozens of children.

Later contacts

The islanders reported that it was not until 27 December 1795 that the first ship after Bounty was seen from the island, but as she did not approach the land, they could not make out to what nation she belonged. A second appeared some time in 1801, but did not attempt to communicate with them. A third came sufficiently near to see their habitations, but did not venture to send a boat ashore.^[20][21]

The American trading ship Topaz, under the command of Mayhew Folger, was the first to visit the island and communicate with the inhabitants when the crew spent 10 hours at Pitcairn in February 1808. A report of Folger's find was forwarded to the Admiralty—which mentioned the discovery and the position of the island at latitude 25° 2' south and longitude 130° west;^[22] however, this rediscovery was not known to Sir Thomas Staines, who commanded a Royal Navy flotilla of two ships (HMS Briton and HMS Tagus), which found the island at 25° 4' S. (by meridian observation) on 17 September 1814. Staines sent a party ashore and wrote a detailed report for the Admiralty.^[20][21][23] In November 2009 a logbook kept by midshipman J.B. Hoodthorp of HMS Briton detailing the first contact with the mutineers was auctioned for over £40,000 by Cheffin's Auction House in Cambridge.^[24]

In 1808, when Topaz reached Pitcairn Island, only John Adams, nine women, and some children still lived. In 1825, Adams was granted amnesty for his mutiny; Pitcairn's capital, Adamstown, is named for him. On 30 November 1838, the Pitcairn Islands (which include the uninhabited islands of Henderson, Ducie and Oeno) were incorporated into the British Empire. In 1856, the British government granted Norfolk Island to the Pitcairners for settlement since population growth was rendering their original refuge uninhabitable.

The Pitcairn Islands are a British Overseas Territory with a population of about 48.^[25] Bounty Day is celebrated on 23 January by Pitcairn Islanders in commemoration of the 1790 burning of the Bounty, and on 8 June as the national holiday on Norfolk Island to commemorate the 1856 arrival of settlers from Pitcairn Island.

Mission details

The details of the voyage of HMAV Bounty are very well documented, largely due to the effort of William Bligh to maintain an accurate log before, during, and after the actual mutiny. Bounty's crew list is also well chronicled, down to and including the names of every seaman on board, something which larger ships in the rating system only occasionally were capable of due to crews in the hundreds whereas the Bounty carried fewer than fifty personnel.

Mission log

• 1787
  • 16 August: William Bligh is ordered to command a breadfruit gathering expedition to Tahiti
  • 3 September: HMAV Bounty launched from the drydock at Deptford
  • 4–9 October: Bounty navigated with a partial crew to an ammunition loading station, south of Deptford
  • 10–12 October: Onload of arms and weapons at Long Reach
  • 15 October – 4 November: Navigated to Spithead for final crew and stores onload
  • 29 November: Made anchor at St Helens, Isle of Wight
  • 23 December: Departed English waters for Tahiti
• 1788
  • 5–10 January: Anchored off Tenerife, Canary Islands
  • 5 February: Crossed equator at 21.50 degrees West
  • 26 February: Marked at 100 leagues from the eastern coast of Brazil
  • 23 March: Arrived Tierra del Fuego
  • 9 April: Entered the Strait of Magellan
  • 25 April: Abandoned attempt to round Cape Horn and turned east
  • 22 May: Within sight of the Cape of Good Hope
  • 24 May – 29 June: Anchored at Simon's Bay
  • 28 July: Within sight of Saint Paul's Island, west of Van Diemen's Land
  • 20 August – 2 September: Anchored Van Diemen's Land
  • 19 September: Past the southern tip of New Zealand
  • 26 October: Arrived Tahiti
  • 25 December: Shifted moores to Owharre Harbor, Huahine, Society Islands
• 1789
  • 4 April: Weighed anchor from Huahine
  • 23–25 April: Anchored for provisions off Annamooka (Tonga)
  • 26 April: Departed Annamooka for the West Indies
  • 28 April: Mutiny on the Bounty. Captain Bligh and loyal crew members set adrift in Bounty's launch
• From this point, Captain Bligh's mission log reflects the voyage of the Bounty launch towards the Dutch East Indies.
  • 29 April: Bounty launch arrives at Tofua
  • 2 May: Bounty launch castaways flee Tofua after being attacked by natives
  • 28 May: Landfall on a small island north of New Hebrides. Named "Restoration Island" by Captain Bligh
  • 30–31 May: Bounty launch transits to a second nearby island, named "Sunday Island"
  • 1–2 June: Bounty launch transits forty two miles to a third island, named "Turtle Island"
  • 3 June: Bounty launch sails into the open ocean towards Australia
  • 13 June: Bounty launch lands at Timor
  • 14 June: Launch castaways circle Timor and land at Coupang. Mutiny is reported to Dutch authorities
• Captain Bligh's mission log from this point reflects his return to England onboard various merchant vessels and sailing ships.
  • 20 August – 10 September: Sailed via schooner to Pasuruan, Java
  • 11–12 September: In transit to Surabaya
  • 15–17 September: In transit to the town of Crissey, Madura Strait
  • 18–22 September: In transit to Semarang
  • 26 September – 1 October: In transit to Batavia (Jakarta)
  • 16 October: Sailed for Europe on board the Dutch packet SS Vlydte
  • 16 December: Arrived Cape of Good Hope
• 1790
  • 13 January: Sailed from Cape of Good Hope for England
  • 13 March: Arrived Portsmouth Harbour

Crew list

Page one of Bligh's list of mutineers – starting with Fletcher Christian.

In the 18th century Royal Navy, rank and position on board ship was defined by a mix of two hierarchies, an official hierarchy of ranks (commissioned officers, warrant officers, petty officers and seamen) and a conventionally recognized social divide between gentlemen and non-gentlemen. Royal Navy uniforms were often used to denote rank and position on board ships; however, due to the lengthy and isolated voyage of the Bounty, uniforms were not worn daily on board while the ship was underway.

At the top of the official rank hierarchy were the commissioned officers – on a larger warship, the commissioned officers included the captain, several lieutenants to command watches, and the officers commanding the Royal Marines on board the ship. The Bounty, however, carried no marines, and no commissioned officers other than Lieutenant Bligh himself, who served as master and commander of the ship. As he was effectively the captain, he occupied a private cabin.

Next below the commissioned officers came the warrant officers, such as the sailing master, surgeon, boatswain, purser and gunner, who were as likely to be considered skilled tradesmen as gentlemen. As the senior warrant officer, the sailing master and his mates were entitled to berth with the lieutenants in the wardroom (though in this case there were no lieutenants there); other warrant officers berthed in the gunroom. Like commissioned officers, warrant officers had the right of access to the quarterdeck and were immune from punishment by flogging. They held their warrants directly from the navy, and the captain could not alter their rank. Roman Catholics were allowed to serve as warrant officers, but not as commissioned officers.

Below the warrant officers came the petty officers. The petty officers included two separate groups: young gentlemen training to be future commissioned officers, often serving as midshipmen or master's mates, and tradesmen working as skilled assistants to the warrant officers. Although the young gentlemen technically were ratings, holding a rank below warrant officers at the mercy of the captain, as aspiring future commissioned officers they were considered socially superior and were often given a watch (with authority over some warrant officers) or a minor command.

Finally, at the bottom of the hierarchical tree, were the seamen, divided into able seamen and ordinary seamen. Aboard some vessels, an even lower grade existed called landsman, who were seamen-in-training with very little or no naval skill. On board the Bounty, due to the vessel's long and fairly important mission, the only seamen mustered into the crew were able seamen – the ship did not carry any ordinary seamen or landsmen.

Note, however, that the young gentlemen might also be rated as seamen rather than midshipmen on the ship's books; though they were still considered the social superiors of the seamen, petty officers (excluding other young gentlemen) and most warrant officers and could be given authority over them.

In the immediate wake of the mutiny, all but four of the loyal crew joined Captain Bligh in the long boat for the voyage to Timor, and eventually made it safely back to England unless otherwise noted in the table below. Four were detained against their will on Bounty for their needed skills and for lack of space on the long boat. The mutineers first returned to Tahiti, where most of the survivors were later captured by Pandora and taken to England for trial. Nine mutineers continued their flight from the law and eventually settled Pitcairn Island, where all but one died before their fate became known to the outside world.

Crew of the Bounty in 1788–89

Category	Name	Position	Mutiny Status	Notes
Commissioned Officers	Lieutenant William Bligh	Commanding Lieutenant		Also Acting Purser;[26] died in London on 6 December 1817
Wardroom Officers	John Fryer	Sailing Master	loyal	went with Bligh; arrived safely in England; died at Wells-next-the-Sea, Norfolk on 26 May 1817
	Fletcher Christian	Master's Mate promoted mid-cruise to Acting Lieutenant	mutinied	to Pitcairn; killed 20 September 1793
	William Elphinstone	Master's Mate	loyal	went with Bligh; died in Batavia October 1789
	Thomas Huggan	Surgeon		died in Tahiti 9 December 1788 before mutiny
Cockpit Officers	John Hallett	Midshipman	loyal	went with Bligh; arrived safely in England; died 1794 of illness
	Thomas Hayward	Midshipman	loyal	went with Bligh; arrived safely in England; died 1798 in shipwreck
	Thomas Ledward	Surgeon's Mate	loyal	went with Bligh; promoted to Surgeon after death of Thomas Huggan; presumed lost at sea in sinking of Welfare 1789 but reported to have been ship surgeon on HMS Discovery in 1791 and died several years later
	John Samuel	Clerk	loyal	went with Bligh; arrived safely in England
Warrant Officers	William Cole	Boatswain	loyal	went with Bligh; arrived safely in England
	Charles Churchill	Master-at-Arms (Ship's Corporal)	mutinied	to Tahiti; murdered by Matthew Thompson in Tahiti April 1790 prior to trial
	William Peckover	Gunner	loyal	went with Bligh; arrived safely in England
	Joseph Coleman	Armourer	loyal	detained on Bounty against his will; to Tahiti; tried and acquitted
	Peter Linkletter	Quartermaster	loyal	went with Bligh; died in Batavia October 1789
	John Norton	Quartermaster	loyal	went with Bligh; killed by natives in Tofua 2 May 1789
	Lawrence LeBogue	Sailmaker	loyal	went with Bligh; arrived safely in England – did join Bligh on the second breadfruit expedition
	Henry Hillbrandt	Cooper	mutinied	to Tahiti; drowned in irons during wreck of Pandora 29 August 1791
	William Purcell	Carpenter	loyal	went with Bligh; arrived safely in England; reportedly died in Haslar hospital 10 March 1834 – last survivor of the Bounty crew
	David Nelson	Botanist (civilian)	loyal	went with Bligh; died 20 July 1789 at Coupang
Midshipmen mustered as Able Seamen	Peter Heywood	Midshipman	mutinied	detained against will (?) on Bounty; to Tahiti; sentenced to death, but pardoned; aka Roger Byam in novels by Charles Nordhoff and James Norman Hall
	George Stewart	Midshipman	loyal	detained against will on Bounty; to Tahiti; killed after being hit by gangway at wreck of Pandora 29 August 1791
	Robert Tinkler	Midshipman	loyal	went with Bligh; arrived safely in England
	Ned Young	Midshipman	mutinied	to Pitcairn; died 25 December 1800
Petty Officers	James Morrison	Boatswain's Mate	mutinied	stayed on Bounty; to Tahiti; sentenced to death, but pardoned. Lost on HMS Blenheim 1807
	George Simpson	Quartermaster's Mate	loyal	went with Bligh; arrived safely in England
	John Williams	Armourer's Mate	mutinied	to Pitcairn; killed 20 September 1793
	Thomas McIntosh	Carpenter's Mate	loyal	detained against will on Bounty; to Tahiti; tried and acquitted
	Charles Norman	Carpenter's Mate	loyal	detained against will on Bounty; to Tahiti; tried and acquitted
	John Mills	Gunner's Mate	mutinied	to Pitcairn; killed 20 September 1793
	William Muspratt	Tailor	mutinied	to Tahiti; sentenced to death, but released on appeal and pardoned. Died on HMS Bellerophon 1797
	John Smith	Steward	loyal	went with Bligh; arrived safely in England – did join Bligh on the second breadfruit expedition
	Thomas Hall	Cook	loyal	went with Bligh; died from a tropical disease (probably malaria) in Batavia on 11 October 1789
	Richard Skinner	Barber	mutinied	to Tahiti; drowned in irons during wreck of Pandora 29 August 1791
	William Brown	Botanist's Assistant	mutinied	to Pitcairn; killed 20 September 1793
	Robert Lamb	Butcher	loyal	went with Bligh; died at sea en route Batavia to Cape Town
Able Seamen	John Adams	Able Seaman	mutinied	to Pitcairn; pardoned 1825, died 1829; aka Alexander Smith
	Thomas Burkitt	Able Seaman	mutinied	to Tahiti; condemned and hanged 29 October 1792 at Spithead
	Michael Byrne	Able Seaman	loyal	detained against will on Bounty; to Tahiti; tried and acquitted
	Thomas Ellison	Able Seaman	mutinied	to Tahiti; condemned and hanged 29 October 1792 at Spithead
	Isaac Martin	Able Seaman	mutinied	to Pitcairn; killed 20 September 1793
	William McCoy	Able Seaman	mutinied	to Pitcairn; committed suicide 1797/98
	John Millward	Able Seaman	mutinied	to Tahiti; condemned and hanged 29 October 1792 at Spithead
	Matthew Quintal	Able Seaman	mutinied	to Pitcairn; "executed" 1799 by Adams and Young
	John Sumner	Able Seaman	mutinied	to Tahiti; drowned in irons during wreck of Pandora 29 August 1791
	Matthew Thompson	Able Seaman	mutinied	to Tahiti; executed by Tahitians in April 1790 prior to trial after killing Charles Churchill
	James Valentine	Able Seaman		died of scurvy at sea 9 October 1788 prior to mutiny; listed in some texts as an Ordinary Seaman

Crew members' biographical information may be found on the Bounty's Crew Encyclopedia page at the Pitcairn Islands Study Centre (PISC).

Discovery of the wreck

Luis Marden discovered the remains of Bounty in January 1957. After spotting a rudder from the ship in a museum on Fiji, he persuaded his editors and writers to let him dive off Pitcairn Island, where the rudder had been found. Despite the warnings of one islander – "Man, you gwen be dead as a hatchet!"^[27] – Marden dived for several days in the dangerous swells near the island, and found the remains of the fabled ship. He subsequently met with Marlon Brando to counsel him on his role as Fletcher Christian in the 1962 film Mutiny on the Bounty. Later in life, Marden wore cuff links made of nails from the Bounty.

Recreation of the voyage

In April 2010, 221 years after the original voyage, a crew recreating Captain William Bligh's epic voyage after the mutiny on Bounty was set adrift in Tongan waters.^[28] The expedition eschewed the use of modern technology including compasses and toilet paper, and only took the same provisions as were aboard the original ship. The expedition lasted 48 days – one day longer than the original voyage – and was led by Australian adventurer Don McIntyre on board the sailing ship the Talisker Bounty.^[29][30]

Bounty on postage stamps

• Pitcairn Island's first postage stamps were issued on 15 October 1940^[31] with a portrait of the ship entitled "H.M. Armed Vessel Bounty" on the 6d stamp.
• The third definitive issue of 1964 depicted "H.M. Armed Vessel Bounty" on the 1d denomination, changed to 1 cent in 1967.
• In 1976, Bounty was shown as "H.M.S. Bounty" on the 10c stamp.
• Bicentenary Sheetlets and first day covers were issued in 1990 depicting Bounty as "HMAV Bounty".
• In 2004, a set of stamps and first day covers were issued to celebrate "HMAV Bounty", the 1979 replica then based in Sydney.
• In 2007, a set of stamps and first day covers were issued to celebrate "HMS Bounty", the 1962 USA-based replica.

In popular culture

Actor Charles Laughton as Bligh in Mutiny on the Bounty (1935)

The story of the mutiny has been adapted numerous times to the page, the screen, and the stage.
Although William Bligh has frequently been portrayed as a middle-aged man in stage and screen productions about the Bounty, he was thirty-four years old at the time of the mutiny, having been born in 1754.

• Mary Russell Mitford wrote her poem "Christina, the Maid of the South Seas" in 1811, following the 1810 publication of Captain Mayhew Folger's rediscovery of Pitcairn.
• Pitcairn's Island: A New Melo Dramatic Ballet of Action, opened in Drury Lane in April 1816, following publication in the Naval Chronicle of an account of the 1814 visit to Pitcairn of Captain Sir Thomas Staines, of the Briton, and Captain Philip Pipon, of the Tagus.
• Lord Byron published his poem The Island in 1823.
• Sir John Barrow's book, The Eventful History of the Mutiny and Piratical Seizure of H.M.S. Bounty: Its Cause and Consequences (1831), ensured the enduring fame of the Bounty and her people.
• Mark Twain describes the mutiny as background to his story "The Great Revolution in Pitcairn" (1879).
• The Mutineers of the Bounty (original title Les révoltés de la Bounty, 1879) by Jules Verne, based on a work by Gabriel Marcel.^[32]
• R. M. Ballantyne wrote a novel about the mutineers on the Bounty called The Lonely Island (1880).
• The story is also related in Richard Whiteing's 1888 novel The Island.
• A first movie (The Mutiny of the Bounty, 1916) was made in Australia.
• A trilogy of novels, (Mutiny on the 'Bounty '​ (1932), Men Against the Sea, and Pitcairn's Island) by Charles Nordhoff and James Norman Hall (also published in one volume as The Bounty Trilogy), as well as the movies and television shows based on them, relate fictionalized versions of the mutiny.
• The second film version was the Australian film In the Wake of the Bounty (1933), starring Errol Flynn as Fletcher Christian.
• The next movie was Mutiny on the Bounty (1935), which won the Oscar for Best Picture that year. It starred Charles Laughton as Bligh and Clark Gable as Christian.
• On 13 January 1939 Orson Welles' The Campbell Playhouse broadcast a radio dramatization, with Welles starring as Bligh and Joseph Cotten as Christian.
• Another film version of the Mutiny on the Bounty (1962) stars Trevor Howard as Bligh and Marlon Brando as Christian. The 1962 motion picture is generally considered the least historically accurate, with such changes or errors as Christian and Bligh's meeting (and subsequently hating) each other at the first sailing of the Bounty, the mutiny's occurring in the middle of the day sparked by Bligh's order to let a sailor die of ingested saltwater poisoning rather than be given water set aside for the breadfruits, and Fletcher Christian's dying from injuries sustained in the fire aboard Bounty while trying to save the ship.
• Bengt Danielsson, a Kon-Tiki crew member, wrote What Happened on the Bounty in 1962.
• A fifth film, The Bounty (1984), stars Anthony Hopkins as William Bligh and Mel Gibson as Fletcher Christian. This film is generally considered the most historically accurate with some of the scenes reenacted directly from William Bligh's own log.
• Queensland Museum marine archaeology curator Peter Gesner wrote Pandora, an archaeological perspective in 1991 (Qld. Museum Press, Brisbane). A revised and updated edition was published by the Qld. Museum in 2000.
• BBC Radio 4 broadcast an adaptation of the Nordhoff-Hall novel in three parts by Bert Coules in 1996, starring Oliver Reed as William Bligh, Roger Daltrey as Fletcher Christian, Lionel Jeffries, and Linus Roach.
• Australian author Peter Corris wrote a novel called The Journal of Fletcher Christian in 2005.
• The Wettest Stories Ever Told, a 2006 episode of the animated series The Simpsons, features a story based on the mutiny on the Bounty.
• Val McDermid explores the fate of Fletcher Christian in her novel The Grave Tattoo (2007).
• Rasputina wrote the double album Oh Perilous World in 2007 as faux 1930s musical theater about Pitcairnian mutineer life, with thinly veiled, anti-neoconservative allegory.
• John Boyne wrote a novel called Mutiny: A Novel of the Bounty, published in 2008, about the voyage of the Bounty and the mutiny from the perspective of Captain Bligh's young personal valet, John Jacob Turnstile.
• Nicholas Pinhey, a British author, wrote After the Bounty (novel) in 2014, a fictionalised account of the lives of the mutineers once they settled on Pitcairn Island.
• A comic book satire featured Mickey Mouse and Goofy shanghaied by Captain Bligh and taken on his historic and ill-fated voyage.
• On the television series M*A*S*H episode "Rainbow Bridge" Frank Burn's accuses Hawkeye of committing mutiny on a bus he was in command of, to which Hawkeye tells Father Mulcahy "MUTINY ON THE BUS.. It was a B-movie, they couldn't afford a bounty."