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Monday, March 23, 2015

Artificial Satellite


From Wikipedia, the free encyclopedia

NASA's Earth-observing fleet as of June 2012.

An animation depicting the orbits of GPS satellites in medium Earth orbit.

A full-size model of the Earth observation satellite ERS 2

In the context of spaceflight, a satellite is an artificial object which has been intentionally placed into orbit. Such objects are sometimes called artificial satellites to distinguish them from natural satellites such as the Moon.

The world's first artificial satellite, the Sputnik 1, was launched by the Soviet Union in 1957. Since then, thousands of satellites have been launched into orbit around the Earth. Some satellites, notably space stations, have been launched in parts and assembled in orbit. Artificial satellites originate from more than 40 countries and have used the satellite launching capabilities of ten nations. A few hundred satellites are currently operational, whereas thousands of unused satellites and satellite fragments orbit the Earth as space debris. A few space probes have been placed into orbit around other bodies and become artificial satellites to the Moon, Mercury, Venus, Mars, Jupiter, Saturn, Vesta, Eros, Ceres,[1] and the Sun.

Satellites are used for a large number of purposes. Common types include military and civilian Earth observation satellites, communications satellites, navigation satellites, weather satellites, and research satellites. Space stations and human spacecraft in orbit are also satellites. Satellite orbits vary greatly, depending on the purpose of the satellite, and are classified in a number of ways. Well-known (overlapping) classes include low Earth orbit, polar orbit, and geostationary orbit.

About 6,600 satellites have been launched. The latest estimates are that 3,600 remain in orbit.[2] Of those, about 1,000 are operational;[3][4] the rest have lived out their useful lives and are part of the space debris. Approximately 500 operational satellites are in low-Earth orbit, 50 are in medium-Earth orbit (at 20,000 km), the rest are in geostationary orbit (at 36,000 km).[5]

Satellites are propelled by rockets to their orbits. Usually the launch vehicle itself is a rocket lifting off from a launch pad on land. In a minority of cases satellites are launched at sea (from a submarine or a mobile maritime platform) or aboard a plane (see air launch to orbit).

Satellites are usually semi-independent computer-controlled systems. Satellite subsystems attend many tasks, such as power generation, thermal control, telemetry, attitude control and orbit control.

History

Early conceptions

"Newton's cannonball", presented as a "thought experiment" in A Treatise of the System of the World, was the first published mathematical study of the possibility of an artificial satellite.

The first fictional depiction of a satellite being launched into orbit is a short story by Edward Everett Hale, The Brick Moon. The story is serialized in The Atlantic Monthly, starting in 1869.[6][7] The idea surfaces again in Jules Verne's The Begum's Fortune (1879).

Konstantin Tsiolkovsky

In 1903, Konstantin Tsiolkovsky (1857–1935) published Exploring Space Using Jet Propulsion Devices (in Russian: Исследование мировых пространств реактивными приборами), which is the first academic treatise on the use of rocketry to launch spacecraft. He calculated the orbital speed required for a minimal orbit around the Earth at 8 km/s, and that a multi-stage rocket fuelled by liquid propellants could be used to achieve this. He proposed the use of liquid hydrogen and liquid oxygen, though other combinations can be used.

In 1928, Slovenian Herman Potočnik (1892–1929) published his sole book, The Problem of Space Travel — The Rocket Motor (German: Das Problem der Befahrung des Weltraums — der Raketen-Motor), a plan for a breakthrough into space and a permanent human presence there. He conceived of a space station in detail and calculated its geostationary orbit. He described the use of orbiting spacecraft for detailed peaceful and military observation of the ground and described how the special conditions of space could be useful for scientific experiments. The book described geostationary satellites (first put forward by Tsiolkovsky) and discussed communication between them and the ground using radio, but fell short of the idea of using satellites for mass broadcasting and as telecommunications relays.

In a 1945 Wireless World article, the English science fiction writer Arthur C. Clarke (1917–2008) described in detail the possible use of communications satellites for mass communications.[8] Clarke examined the logistics of satellite launch, possible orbits and other aspects of the creation of a network of world-circling satellites, pointing to the benefits of high-speed global communications. He also suggested that three geostationary satellites would provide coverage over the entire planet.

The US military studied the idea of what was referred to as the earth satellite vehicle when Secretary of Defense James Forrestal made a public announcement on December 29, 1948, that his office was coordinating that project between the various services.[9]

Artificial satellites


Sputnik 1: The first artificial satellite to orbit Earth.

The first artificial satellite was Sputnik 1, launched by the Soviet Union on October 4, 1957, and initiating the Soviet Sputnik program, with Sergei Korolev as chief designer (there is a crater on the lunar far side which bears his name). This in turn triggered the Space Race between the Soviet Union and the United States.

Sputnik 1 helped to identify the density of high atmospheric layers through measurement of its orbital change and provided data on radio-signal distribution in the ionosphere. The unanticipated announcement of Sputnik 1's success precipitated the Sputnik crisis in the United States and ignited the so-called Space Race within the Cold War.

Sputnik 2 was launched on November 3, 1957 and carried the first living passenger into orbit, a dog named Laika.[10]

In May, 1946, Project RAND had released the Preliminary Design of an Experimental World-Circling Spaceship, which stated, "A satellite vehicle with appropriate instrumentation can be expected to be one of the most potent scientific tools of the Twentieth Century."[11] The United States had been considering launching orbital satellites since 1945 under the Bureau of Aeronautics of the United States Navy. The United States Air Force's Project RAND eventually released the above report, but did not believe that the satellite was a potential military weapon; rather, they considered it to be a tool for science, politics, and propaganda. In 1954, the Secretary of Defense stated, "I know of no American satellite program."[12] In February 1954 Project RAND released "Scientific Uses for a Satellite Vehicle," written by R.R. Carhart.[13] This expanded on potential scientific uses for satellite vehicles and was followed in June 1955 with "The Scientific Use of an Artificial Satellite," by H.K. Kallmann and W.W. Kellogg.[14]

In the context of activities planned for the International Geophysical Year (1957–58), the White House announced on July 29, 1955 that the U.S. intended to launch satellites by the spring of 1958. This became known as Project Vanguard. On July 31, the Soviets announced that they intended to launch a satellite by the fall of 1957.

Following pressure by the American Rocket Society, the National Science Foundation, and the International Geophysical Year, military interest picked up and in early 1955 the Army and Navy were working on Project Orbiter, two competing programs: the army's which involved using a Jupiter C rocket, and the civilian/Navy Vanguard Rocket, to launch a satellite. At first, they failed: initial preference was given to the Vanguard program, whose first attempt at orbiting a satellite resulted in the explosion of the launch vehicle on national television. But finally, three months after Sputnik 2, the project succeeded; Explorer 1 became the United States' first artificial satellite on January 31, 1958.[15]

In June 1961, three-and-a-half years after the launch of Sputnik 1, the Air Force used resources of the United States Space Surveillance Network to catalog 115 Earth-orbiting satellites.[16]

Early satellites were constructed as "one-off" designs. With growth in geosynchronous (GEO) satellite communication, multiple satellites began to be built on single model platforms called satellite buses. The first standardized satellite bus design was the HS-333 GEO commsat, launched in 1972.

The largest artificial satellite currently orbiting the Earth is the International Space Station.

1U CubeSat ESTCube-1, developed mainly by the students from the University of Tartu, carries out a tether deployment experiment on the low Earth orbit.

Space Surveillance Network

The United States Space Surveillance Network (SSN), a division of The United States Strategic Command, has been tracking objects in Earth's orbit since 1957 when the Soviets opened the space age with the launch of Sputnik I. Since then, the SSN has tracked more than 26,000 objects. The SSN currently tracks more than 8,000 man-made orbiting objects. The rest have re-entered Earth's atmosphere and disintegrated, or survived re-entry and impacted the Earth. The SSN tracks objects that are 10 centimeters in diameter or larger; those now orbiting Earth range from satellites weighing several tons to pieces of spent rocket bodies weighing only 10 pounds. About seven percent are operational satellites (i.e. ~560 satellites), the rest are space debris.[17] The United States Strategic Command is primarily interested in the active satellites, but also tracks space debris which upon reentry might otherwise be mistaken for incoming missiles.
A search of the NSSDC Master Catalog at the end of October 2010 listed 6,578 satellites launched into orbit since 1957, the latest being Chang'e 2, on 1 October 2010.[18]

Non-military satellite services

There are three basic categories of non-military satellite services:[19]

Fixed satellite services

Fixed satellite services handle hundreds of billions of voice, data, and video transmission tasks across all countries and continents between certain points on the Earth's surface.

Mobile satellite systems

Mobile satellite systems help connect remote regions, vehicles, ships, people and aircraft to other parts of the world and/or other mobile or stationary communications units, in addition to serving as navigation systems.

Scientific research satellites (commercial and noncommercial)

Scientific research satellites provide meteorological information, land survey data (e.g. remote sensing), Amateur (HAM) Radio, and other different scientific research applications such as earth science, marine science, and atmospheric research.

Types


MILSTAR: A communication satellite

International Space Station as seen from Space
  • Space stations are man-made orbital structures that are designed for human beings to live on in outer space. A space station is distinguished from other manned spacecraft by its lack of major propulsion or landing facilities. Space stations are designed for medium-term living in orbit, for periods of weeks, months, or even years.

Orbit types

Various earth orbits to scale; cyan represents low earth orbit, yellow represents medium earth orbit, the black dashed line represents geosynchronous orbit, the green dash-dot line the orbit of Global Positioning System (GPS) satellites, and the red dotted line the orbit of the International Space Station (ISS).

The first satellite, Sputnik 1, was put into orbit around Earth and was therefore in geocentric orbit. By far this is the most common type of orbit with approximately 2,465[citation needed] artificial satellites orbiting the Earth. Geocentric orbits may be further classified by their altitude, inclination and eccentricity.

The commonly used altitude classifications of geocentric orbit are Low Earth orbit (LEO), Medium Earth orbit (MEO) and High Earth orbit (HEO). Low Earth orbit is any orbit below 2,000 km. Medium Earth orbit is any orbit between 2,000 km-35,786 km. High Earth orbit is any orbit higher than 35,786 km.

Centric classifications

The general structure of a satellite is that it is connected to the earth stations that are present on the ground and connected through terrestrial links.

Altitude classifications


Orbital Altitudes of several significant satellites of earth.

Inclination classifications

  • Inclined orbit: An orbit whose inclination in reference to the equatorial plane is not zero degrees.
    • Polar orbit: An orbit that passes above or nearly above both poles of the planet on each revolution. Therefore it has an inclination of (or very close to) 90 degrees.
    • Polar sun synchronous orbit: A nearly polar orbit that passes the equator at the same local time on every pass. Useful for image taking satellites because shadows will be nearly the same on every pass.

Eccentricity classifications

  • Circular orbit: An orbit that has an eccentricity of 0 and whose path traces a circle.
    • Hohmann transfer orbit: An orbit that moves a spacecraft from one approximately circular orbit, usually the orbit of a planet, to another, using two engine impulses. The perihelion of the transfer orbit is at the same distance from the Sun as the radius of one planet's orbit, and the aphelion is at the other. The two rocket burns change the spacecraft's path from one circular orbit to the transfer orbit, and later to the other circular orbit. This maneuver was named after Walter Hohmann.
  • Elliptic orbit: An orbit with an eccentricity greater than 0 and less than 1 whose orbit traces the path of an ellipse.
    • Geosynchronous transfer orbit: An elliptic orbit where the perigee is at the altitude of a Low Earth orbit (LEO) and the apogee at the altitude of a geosynchronous orbit.
    • Geostationary transfer orbit: An elliptic orbit where the perigee is at the altitude of a Low Earth orbit (LEO) and the apogee at the altitude of a geostationary orbit.
    • Molniya orbit: A highly elliptic orbit with inclination of 63.4° and orbital period of half of a sidereal day (roughly 12 hours). Such a satellite spends most of its time over two designated areas of the planet (specifically Russia and the United States).
    • Tundra orbit: A highly elliptic orbit with inclination of 63.4° and orbital period of one sidereal day (roughly 24 hours). Such a satellite spends most of its time over a single designated area of the planet.

Synchronous classifications

  • Synchronous orbit: An orbit where the satellite has an orbital period equal to the average rotational period (earth's is: 23 hours, 56 minutes, 4.091 seconds) of the body being orbited and in the same direction of rotation as that body. To a ground observer such a satellite would trace an analemma (figure 8) in the sky.
  • Semi-synchronous orbit (SSO): An orbit with an altitude of approximately 20,200 km (12,600 mi) and an orbital period equal to one-half of the average rotational period (earth's is approximately 12 hours) of the body being orbited
  • Geosynchronous orbit (GSO): Orbits with an altitude of approximately 35,786 km (22,236 mi). Such a satellite would trace an analemma (figure 8) in the sky.
  • Areosynchronous orbit: A synchronous orbit around the planet Mars with an orbital period equal in length to Mars' sidereal day, 24.6229 hours.
  • Areostationary orbit (ASO): A circular areosynchronous orbit on the equatorial plane and about 17000 km (10557 miles) above the surface. To an observer on the ground this satellite would appear as a fixed point in the sky.
  • Heliosynchronous orbit: A heliocentric orbit about the Sun where the satellite's orbital period matches the Sun's period of rotation. These orbits occur at a radius of 24,360 Gm (0.1628 AU) around the Sun, a little less than half of the orbital radius of Mercury.

Special classifications

Pseudo-orbit classifications

  • Horseshoe orbit: An orbit that appears to a ground observer to be orbiting a certain planet but is actually in co-orbit with the planet. See asteroids 3753 (Cruithne) and 2002 AA29.
  • Exo-orbit: A maneuver where a spacecraft approaches the height of orbit but lacks the velocity to sustain it.
  • Lunar transfer orbit (LTO)
  • Prograde orbit: An orbit with an inclination of less than 90°. Or rather, an orbit that is in the same direction as the rotation of the primary.
  • Retrograde orbit: An orbit with an inclination of more than 90°. Or rather, an orbit counter to the direction of rotation of the planet. Apart from those in sun-synchronous orbit, few satellites are launched into retrograde orbit because the quantity of fuel required to launch them is much greater than for a prograde orbit. This is because when the rocket starts out on the ground, it already has an eastward component of velocity equal to the rotational velocity of the planet at its launch latitude.
  • Halo orbit and Lissajous orbit: Orbits "around" Lagrangian points.

Satellite subsystems

The satellite's functional versatility is imbedded within its technical components and its operations characteristics. Looking at the "anatomy" of a typical satellite, one discovers two modules.[19] Note that some novel architectural concepts such as Fractionated Spacecraft somewhat upset this taxonomy.

Spacecraft bus or service module

The bus module consists of the following subsystems:
  • The Structural Subsystem
The structural subsystem provides the mechanical base structure with adequate stiffness to withstand stress and vibrations experienced during launch, maintain structural integrity and stability while on station in orbit, and shields the satellite from extreme temperature changes and micro-meteorite damage.
  • The Telemetry Subsystem (aka Command and Data Handling, C&DH)
The telemetry subsystem monitors the on-board equipment operations, transmits equipment operation data to the earth control station, and receives the earth control station's commands to perform equipment operation adjustments.
  • The Power Subsystem
The power subsystem consists of solar panels to convert solar energy into electrical power, regulation and distribution functions, and batteries that store power and supply the satellite when it passes into the Earth's shadow.
Nuclear power sources (Radioisotope thermoelectric generator have also been used in several successful satellite programs including the Nimbus program (1964–1978).[23]
The thermal control subsystem helps protect electronic equipment from extreme temperatures due to intense sunlight or the lack of sun exposure on different sides of the satellite's body (e.g. Optical Solar Reflector)
  • The Attitude and Orbit Control Subsystem
The attitude and orbit control subsystem consists of sensors to measure vehicle orientation; control laws embedded in the flight software; and actuators (reaction wheels, thrusters) to apply the torques and forces needed to re-orient the vehicle to a desired attitude, keep the satellite in the correct orbital position and keep antennas positioning in the right directions.

Communication payload

The second major module is the communication payload, which is made up of transponders. A transponder is capable of :
  • Receiving uplinked radio signals from earth satellite transmission stations (antennas).
  • Amplifying received radio signals
  • Sorting the input signals and directing the output signals through input/output signal multiplexers to the proper downlink antennas for retransmission to earth satellite receiving stations (antennas).

End of life

When satellites reach the end of their mission, satellite operators have the option of de-orbiting the satellite, leaving the satellite in its current orbit or moving the satellite to a graveyard orbit. Historically, due to budgetary constraints at the beginning of satellite missions, satellites were rarely designed to be de-orbited. One example of this practice is the satellite Vanguard 1. Launched in 1958, Vanguard 1, the 4th manmade satellite put in Geocentric orbit, was still in orbit as of August 2009.[24]

Instead of being de-orbited, most satellites are either left in their current orbit or moved to a graveyard orbit.[25] As of 2002, the FCC requires all geostationary satellites to commit to moving to a graveyard orbit at the end of their operational life prior to launch.[26] In cases of uncontrolled de-orbiting, the major variable is the solar flux, and the minor variables the components and form factors of the satellite itself, and the gravitational perturbations generated by the Sun and the Moon (as well as those exercised by large mountain ranges, whether above or below sea level).
The nominal breakup altitude due to aerodynamic forces and temperatures is 78 km, with a range between 72 and 84 km. Solar panels, however, are destroyed before any other component at altitudes between 90 and 95 km.[27]

Launch-capable countries

This list includes countries with an independent capability of states to place satellites in orbit, including production of the necessary launch vehicle. Note: many more countries have the capability to design and build satellites but are unable to launch them, instead relying on foreign launch services. This list does not consider those numerous countries, but only lists those capable of launching satellites indigenously, and the date this capability was first demonstrated. The list include multi-national state organization ESA but does not include private consortiums.
First launch by country
Order Country Date of first launch Rocket Satellite
1  Soviet Union 4 October 1957 Sputnik-PS Sputnik 1
2  United States 1 February 1958 Juno I Explorer 1
3  France 26 November 1965 Diamant-A Astérix
4  Japan 11 February 1970 Lambda-4S Ōsumi
5  China 24 April 1970 Long March 1 Dong Fang Hong I
6  United Kingdom 28 October 1971 Black Arrow Prospero
7  India 18 July 1980 SLV Rohini D1
8  Israel 19 September 1988 Shavit Ofeq 1
- [1]  Russia 21 January 1992 Soyuz-U Kosmos 2175
- [1]  Ukraine 13 July 1992 Tsyklon-3 Strela
9  Philippines 20 August 1997 Long March 3B Agila 2
10  Iran 2 February 2009 Safir-1 Omid
11  North Korea 12 December 2012 Unha-3 Kwangmyŏngsŏng-3 Unit 2

Attempted first launches

  • United States tried in 1957 to launch the first satellite by own launcher before successfully completing a launch in 1958.
  • China tried in 1969 to launch the first satellite by own launcher before successfully completing a launch in 1970.
  • India, after launching the first national satellite by foreign launcher in 1975, tried in 1979 to launch the first satellite by own launcher before succeeding in 1980.
  • Iraq have claimed orbital launch of warhead in 1989, but this claim was later disproved.[31]
  • Brazil, after launch of first national satellite by foreign launcher in 1985, tried to launched the satellites by own VLS 1 launcher three times in 1997, 1999, 2003 but all were unsuccessful.
  • North Korea claimed a launch of Kwangmyŏngsŏng-1 and Kwangmyŏngsŏng-2 satellites in 1998 and 2009, but U.S., Russian and other officials and weapons experts later reported that the rockets failed to send a satellites into orbit, if that was the goal. The United States, Japan and South Korea believe this was actually a ballistic missile test, which is a claim also made after North Korea's 1998 satellite launch, and later rejected.[by whom?] The first (April 2012) launch of Kwangmyŏngsŏng-3 was unsuccessful, a fact publicly recognized by the DPRK. However, the December 2012 launch of the "second version" of Kwangmyŏngsŏng-3 was successful, putting the DPRK's first confirmed satellite into orbit.
  • South Korea (Korea Aerospace Research Institute), after launching their first national satellite by foreign launcher in 1992, unsuccessfully tried to launch a first KSLV(Naro)-1 own launcher (created with assistance of Russia) in 2009 and 2010 until success was achieved in 2013 by Naro-3.
  • First European multi-national state organization ELDO tried to make the orbital launches at Europa I and Europa II rockets in 1968-1970 and 1971 but stopped operation after fails.

Other notes

Launch capable private entities

  • Private firm Orbital Sciences Corporation, with launches since 1982, continues very successful launches of its Minotaur, Pegasus, Taurus and Antares rocket programs.
  • On September 28, 2008, late comer and private aerospace firm SpaceX successfully launched its Falcon 1 rocket into orbit. This marked the first time that a privately built liquid-fueled booster was able to reach orbit.[32] The rocket carried a prism shaped 1.5 m (5 ft) long payload mass simulator that was set into orbit. The dummy satellite, known as Ratsat, will remain in orbit for between five and ten years before burning up in the atmosphere.[32]
A few other private companies are capable of sub-orbital launches.

First satellites of countries

First satellites of countries including launched indigenously or by help of other[33]
Country Year of first launch First satellite Payloads in orbit as of Jan 2013[34][needs update]
 Soviet Union
( Russia)
1957
(1992)
Sputnik 1
(Kosmos 2175)
1457
 United States 1958 Explorer 1 1110
 United Kingdom 1962 Ariel 1 0030
 Canada 1962 Alouette 1 0034
 Italy 1964 San Marco 1 0022
 France 1965 Astérix 0057
 Australia 1967 WRESAT 0012
 Germany 1969 Azur 0042
 Japan 1970 Ōsumi 0134
 China 1970 Dong Fang Hong I 0140
 Netherlands 1974 ANS 0004
 Spain 1974 Intasat 0009
 India 1975 Aryabhata 0054
 Indonesia 1976 Palapa A1 0012
 Czechoslovakia 1978 Magion 1 0004
 Bulgaria 1981 Intercosmos Bulgaria 1300 0001
 Saudi Arabia 1985 Arabsat-1A 0012
 Brazil 1985 Brasilsat A1 0013
 Mexico 1985 Morelos 1 0007
 Sweden 1986 Viking 0011
 Israel 1988 Ofeq 1 00011
 Luxembourg 1988 Astra 1A 005
 Argentina 1990 Lusat[35] 009
 Hong Kong 1990 AsiaSat 1 0009
 Pakistan 1990 Badr-1 0003
 South Korea 1992 Kitsat A 0011
 Portugal 1993 PoSAT-1 0001
 Thailand 1993 Thaicom 1 0007
 Turkey 1994 Turksat 1B 0008
 Ukraine 1995 Sich-1 0006
 Malaysia 1996 MEASAT 0006
 Norway 1997 Thor 2 0003
 Philippines 1997 Mabuhay 1 0002
 Egypt 1998 Nilesat 101 0004
 Chile 1998 FASat-Bravo 0002
 Singapore 1998 ST-1[36][37] 0003
 Taiwan 1999 ROCSAT-1 0008
 Denmark 1999 Ørsted 0004
 South Africa 1999 SUNSAT 0002
 United Arab Emirates 2000 Thuraya 1 0006
 Morocco 2001 Maroc-Tubsat 0001
 Tonga[38] 2002 Esiafi 1 (former Comstar D4) 1
 Algeria 2002 Alsat 1 0001
 Greece 2003 Hellas Sat 2 0002
 Cyprus 2003 Hellas Sat 2 0002
 Nigeria 2003 Nigeriasat 1 0004
 Iran 2005 Sina-1 0001
 Kazakhstan 2006 KazSat 1 0002
 Colombia 2007 Libertad 1 0001
 Mauritius 2007 Rascom-QAF 1 0002
 Vietnam 2008 Vinasat-1 0003
 Venezuela 2008 Venesat-1 0002
  Switzerland 2009 SwissCube-1[39] 0002
 Isle of Man 2011 ViaSat-1 0001
 Poland[40][41] 2012 PW-Sat 00002
 Hungary 2012 MaSat-1 0001
 Romania 2012 Goliat[42] 0001
 Belarus 2012 BKA (BelKA-2)[43] N/A
 North Korea 2012 Kwangmyŏngsŏng-3 Unit 2 1
 Azerbaijan 2013 Azerspace[44] 1
 Austria 2013 TUGSAT-1/UniBRITE[45][46] 2
 Bermuda[47] 2013 Bermudasat 1 (former EchoStar VI) 1
 Ecuador 2013 NEE-01 Pegaso 1
 Estonia 2013 ESTCube-1 1
 Jersey 2013 O3b-1,-2,-3,-4 4
 Qatar 2013 Es'hailSat1 1
 Peru 2013 PUCPSAT-1[48] 1
 Bolivia 2013 TKSat-1 1
 Lithuania 2014 LituanicaSAT-1 and LitSat-1 2
 Uruguay 2014 Antelsat 1
 Iraq 2014 Tigrisat[49] 1

  orbital launch and satellite operation
  satellite operation, launched by foreign supplier
  satellite in development
  orbital launch project at advanced stage or indigenous ballistic missiles deployed

While Canada was the third country to build a satellite which was launched into space,[50] it was launched aboard a U.S. rocket from a U.S. spaceport. The same goes for Australia, who launched first satellite involved a donated U.S. Redstone rocket and U.S. support staff as well as a joint launch facility with the United Kingdom.[51] The first Italian satellite San Marco 1 launched on 15 December 1964 on a U.S. Scout rocket from Wallops Island (VA, USA) with an Italian Launch Team trained by NASA.[52] By similar occasions, almost all further first national satellites was launched by foreign rockets.

Attempted first satellites

  •  USA tried unsuccessfully to launch its first satellite in 1957; they were successful in 1958.
  •  China tried unsuccessfully to launch its first satellite in 1969; they were successful in 1970.
  •  Iraq under Saddam fulfilled in 1989 an unconfirmed launch of warhead on orbit by developed Iraqi vehicle that intended to put later the 75-kg first national satellite Al-Ta’ir, also developed.[53][54]
  •  Chile tried unsuccessfully in 1995 to launch its first satellite FASat-Alfa by foreign rocket; in 1998 they were successful.†
  •  North Korea has tried in 1998, 2009, 2012 to launch satellites, first successful launch on 12 December 2012.[55]
  •  Libya since 1996 developed the own national Libsat satellite project including telecommunication and remote sensing aims[56] that was postponed after fall of Gaddafi.
  •  Belarus tried unsuccessfully in 2006 to launch its first satellite BelKA by foreign rocket.†
†-note: Both Chile and Belarus used Russian companies as principal contractors to build their satellites, they used Russian-Ukrainian manufactured rockets and launched either from Russia or Kazakhstan.

Planned first satellites

  •  Afghanistan announced in April 2012 that it is planning to launch its first communications satellite to the orbital slot it has been awarded. The satellite Afghansat 1 was expected to be obtained by a Eutelsat commercial company in 2014.[57][58]
  •  Angola will have the first telecommunication satellite AngoSat-1 that was ordered in Russia at 2009 for $400 millions, started to construction at the and of 2013 and planning for launch in November 2016.[59]
  •  Armenia in 2012 founded Armcosmos company[60] and announced an intenton to have the first telecommunication satellite ArmSat. The investments estimates as $250 million and country selecting the contractor for building within 4 years the satellite amongst Russia, China and Canada[61][62][63]
  •  Bangladesh announced in 2009 that it intends to launch its first satellite into space by 2011.[64]
  •  Belgium's first nano-satellite OUFTI-1 within European University program CubeSat QB50 for test radio protocol in space is under construction in University of Liege.[65]
  •  Cambodia's Royal Group plans to purchase for $250–350 million and launch in the beginning of 2013 the telecommunication satellite.[66]
  •  Democratic Republic of the Congo ordered at November 2012 in China (Academy of Space Technology (CAST) and Great Wall Industry Corporation (CGWIC)) the first telecommunication satellite CongoSat-1 which will be built on DFH-4 satellite bus platform and will be launched in China till the end of 2015.[67]
  •  Croatia has a goal to construct a satellite by 2013–2014. Launch into Earth orbit would be done by a foreign provider.[68]
  •  Ethiopian Space Science Society [69] planning the QB50-family research CubeSat ET-SAT by help of Belgian Von Karman Institute till 2015[70] and the small (20–25 kg) Earth observation and remote sensing satellite Ethosat 1 by help of Finnish Space Technology and Science Group till 2019.[71]
  •  Finland's Aalto-1 Cusesat-satellite (3U) with solar panels is a funded by student nano-satellite project of Aalto University and Finnish Meteorological Institute [2]. When launched (plan was to 2013), it would be the first Finnish satellite. Launch has been procured for the summer 2015.
  •  Ghana plans to order in UK and Italy and launch within 2020 the first Earth observation satellite Ghanasat-1.[72]
  •  Ireland's team of Dublin Institute of Technology intends to launch the first Irish satellite within European University program CubeSat QB50.[73]
  •  Jordan's first satellite to be the private amateur pocketqube SunewnewSat.[74][75][76]
  •  Kenyan University of Nairobi has plans to create the microsatellite KenyaSat by help of UK's University of Surrey.[77]
  •  Laos announced that its first satellite will be telecommunication and will be built and launched in 2013 for $250 million by China Asia-Pacific Mobile Communications Company (China-APMT).[78]
  •  Latvia's the 5 kg nano-satellite Venta-1 is built in Latvia in cooperation with the German engineers. The data received from satellite will be received and processed in Irbene radioastronomical centre (Latvia); satellite will have software defined radio capabilities. "Venta-1" will serve mainly as a means for education in Ventspils University College with additional functions, including an automatic system of identification of the ships of a sailing charter developed by OHB-System AG. The launch of the satellite was planned for the end of 2009 using the Indian carrier rocket. Due to the financial crisis the launch has been postponed until late 2011.[79] Started preparations to produce the next satellite "Venta-2".
  •  Moldova's first remote sensing satellite plans to start in 2013 by Space centre at national Technical University.[80]
  •  Mongolia's National Remote Sensing Center of Mongolia plans to order the communication satellite in Japan, Mongolian Academy of Sciences schedules to launch the first national experimental satellite Mongolsat by US launcher in the first quarter of 2013.[81]
  •  Myanmar plans to purchase for $200 million the own telecommunication satellite.[82]
  •    Nepal stated that planning to launch of own telecommunication satellite before 2015 by help of India or China.[83][84][85]
  •  New Zealand's private Satellite Opportunities company since 2005 plans to launch in 2010 or later a commercial satellite NZLSAT for $200 million.[86] Radio enthusiasts federation at Massey University [3] since 2003 hopes for $400,000 to launch a nano-satellite KiwiSAT to relay a voice and data signals[87] Also another RocketLab company works under suborbital space launcher and may use a further version of one to launch into low polar orbit a nano-satellite.[88]
  •  Nicaragua ordered for $254 million at November 2013 in China the first telecommunication satellite Nicasat-1 (to be built at DFH-4 satellite bus platform by CAST and CGWIC), that planning to launch in China at 2016.[89]
  •  Paraguay under new Aaepa airspace agency plans first Eart observation satellite.[90][91]
  •  Serbia's first satellite Tesla-1 was designed, developed and assembled by nongovermental organisations in 2009 but still remains unlaunched.
  •  Slovenia's Earth observation microsatellite for the Slovenian Centre of Excellence for Space Sciences and Technologies (Space-SI) now under development for $2 million since 2010 by University of Toronto Institute for Aerospace Studies – Space Flight Laboratory (UTIAS – SFL) and planned to launch in 2015-2016.[92][93]
  •  Sri Lanka has a goal to construct two satellites beside of rent the national SupremeSAT payload in Chinese satellites. Sri Lankan Telecommunications Regulatory Commission has signed an agreement with Surrey Satellite Technology Ltd to get relevant help and resources. Launch into Earth orbit would be done by a foreign provider.[94][95]
  •  Syrian Space Research Center developing CubeSat-like small first national satellite since 2008.[96]
  •  Tunisia is developing its first satellite, ERPSat01. Consisting of a CubeSat of 1 kg mass, it will be developed by the Sfax School of Engineering. ERPSat satellite is planned to be launched into orbit in 2013.[97]
  •  Turkmenistan's new National Space Agency plans to launch in 2015 by SpaceX rocket its first telecommunication satellite Turkmensat 1 built by Italian Thales Alenia Space.[98][99][100]
  •  Uzbekistan's State Space Research Agency (UzbekCosmos) announced in 2001 about intention of launch in 2002 first remote sensing satellite.[101] Later in 2004 was stated that two satellites (remote sensing and telecommunication) will be built by Russia for $60–70 million each[102]

Attacks on satellites

In recent times[timeframe?], satellites have been hacked by militant organizations to broadcast propaganda and to pilfer classified information from military communication networks.[103][104]
For testing purposes, satellites in low earth orbit have been destroyed by ballistic missiles launched from earth.
Russia, the United States and China have demonstrated the ability to eliminate satellites.[105] In 2007 the Chinese military shot down an aging weather satellite,[105] followed by the US Navy shooting down a defunct spy satellite in February 2008.[106]

Jamming

Due to the low received signal strength of satellite transmissions, they are prone to jamming by land-based transmitters. Such jamming is limited to the geographical area within the transmitter's range. GPS satellites are potential targets for jamming,[107][108] but satellite phone and television signals have also been subjected to jamming.[109][110]
Also, it is trivial to transmit a carrier radio signal to a geostationary satellite and thus interfere with the legitimate uses of the satellite's transponder. It is common for Earth stations to transmit at the wrong time or on the wrong frequency in commercial satellite space, and dual-illuminate the transponder, rendering the frequency unusable. Satellite operators now have sophisticated monitoring that enables them to pinpoint the source of any carrier and manage the transponder space effectively.[citation needed]

Satellite services


Natural satellite


From Wikipedia, the free encyclopedia

A natural satellite, or moon, is a celestial body that orbits another body (a planet, dwarf planet, or small Solar System body), which is called its primary, and that is not artificial. There are 173 known natural satellites orbiting planets in the Solar System,[1][2] as well as eight known to orbit IAU-listed dwarf planets.[3] As of January 2012, over 200 minor-planet moons have been discovered.[4] There are 76 known objects in the asteroid belt with satellites (five with two each), four Jupiter trojans, 39 near-Earth objects (two with two satellites each), and 14 Mars-crossers.[4] There are also 84 known natural satellites of trans-Neptunian objects.[4] Some 150 additional small bodies have been observed within the rings of Saturn, but only a few were tracked long enough to establish orbits. Planets around other stars are likely to have satellites as well, and although numerous candidates have been detected to date, none have yet been confirmed.

Of the inner planets, Mercury and Venus have no natural satellites; Earth has one large natural satellite, known as the Moon; and Mars has two tiny natural satellites, Phobos and Deimos. The giant planets have extensive systems of natural satellites, including half a dozen comparable in size to Earth's Moon: the four Galilean moons, Saturn's Titan, and Neptune's Triton. Saturn has an additional six mid-sized natural satellites massive enough to have achieved hydrostatic equilibrium, and Uranus has five. It has been suggested that some satellites may potentially harbour life,[5] though there is currently no direct evidence of life.

The Earth–Moon system is unique in that the ratio of the mass of the Moon to the mass of Earth is much greater than that of any other natural-satellite–planet ratio in the Solar System (although there are minor-planet systems with even greater ratios, notably the PlutoCharon system).

Among the dwarf planets, Ceres and Makemake have no known natural satellites. Pluto has the relatively large natural satellite Charon and four smaller natural satellites.[6] Haumea has two natural satellites, and Eris has one. The Pluto–Charon system is unusual in that the center of mass lies in open space between the two, a characteristic sometimes associated with a double-planet system.

Nineteen natural satellites are large enough to be round, and one,
Saturn's moon, Titan, has a substantial atmosphere.

Origin and orbital characteristics


Two moons: Saturn's natural satellite Dione occults Enceladus

The natural satellites orbiting relatively close to the planet on prograde, uninclined circular orbits (regular satellites) are generally believed to have been formed out of the same collapsing region of the protoplanetary disk that created its primary. In contrast, irregular satellites (generally orbiting on distant, inclined, eccentric and/or retrograde orbits) are thought to be captured asteroids possibly further fragmented by collisions. Most of the major natural satellites of the Solar System have regular orbits, while most of the small natural satellites have irregular orbits.[7] The Moon[8] and possibly Charon[9] are exceptions among large bodies in that they are believed to have originated by the collision of two large proto-planetary objects (see the giant impact hypothesis). The material that would have been placed in orbit around the central body is predicted to have reaccreted to form one or more orbiting natural satellites. As opposed to planetary-sized bodies, asteroid moons are thought to commonly form by this process. Triton is another exception; although large and in a close, circular orbit, its motion is retrograde and it is thought to be a captured dwarf planet.

Tidal locking

Most regular moons (natural satellites following relatively close and prograde orbits with small orbital inclination and eccentricity) in the Solar System are tidally locked to their respective primaries, meaning that the same side of the natural satellite always faces its planet. The only known exception is Saturn's natural satellite Hyperion, which rotates chaotically because of the gravitational influence of Titan.
In contrast, the outer natural satellites of the giants planet (irregular satellites) are too far away to have become locked. For example, Jupiter's Himalia, Saturn's Phoebe, and Neptune's Nereid have rotation periods in the range of ten hours, whereas their orbital periods are hundreds of days.

Satellites of satellites


Artist impression of Rhea's proposed rings

No "moons of moons" (natural satellites that orbit a natural satellite of another body) are currently known as of 2015. In most cases, the tidal effects of the primary would make such a system unstable.

However, calculations performed after the recent detection[10] of a possible ring system around Saturn's natural satellite Rhea indicate that satellites orbiting Rhea would have stable orbits. Furthermore, the suspected rings are thought to be narrow,[11] a phenomenon normally associated with shepherd moons. However, targeted images taken by the Cassini spacecraft failed to detect any rings associated with Rhea.[12]

It has also been proposed that Saturn's satellite Iapetus possessed a subsatellite in the past; this is one of several hypotheses that have been put forward to account for its equatorial ridge.[13]

Trojan satellites

Two natural satellites are known to have small companions at their L4 and L5 Lagrangian points, sixty degrees ahead and behind the body in its orbit. These companions are called trojan moons, as their orbits are analogous to the Trojan asteroids of Jupiter. The trojan moons are Telesto and Calypso, which are the leading and following companions, respectively, of Tethys; and Helene and Polydeuces, the leading and following companions of Dione.

Asteroid satellites

The discovery of 243 Ida's natural satellite Dactyl in the early 1990s confirmed that some asteroids have natural satellites; indeed, 87 Sylvia has two. Some, such as 90 Antiope, are double asteroids with two comparably sized components.

Shape


The relative masses of the natural satellites of the Solar System. Mimas, Enceladus, and Miranda are too small to be visible at this scale. All the irregularly shaped natural satellites, even added together, would also be too small to be visible.

Neptune's moon Proteus is the largest irregularly shaped natural satellite. All other known natural satellites that are at least the size of Uranus's Miranda have lapsed into rounded ellipsoids under hydrostatic equilibrium, i.e. are "round/rounded satellites". The larger natural satellites, being tidally locked, tend toward ovoid (egg-like) shapes: squat at their poles and with longer equatorial axes in the direction of their primaries (their planets) than in the direction of their motion. Saturn's moon Mimas, for example, has a major axis 9% greater than its polar axis and 5% greater than its other equatorial axis. Methone, another of Saturn's moons, is only around 3 km in diameter and visibly egg-shaped. The effect is smaller on the largest natural satellites, where their own gravity is greater relative to the effects of tidal distortion, especially those that orbit less massive planets or, as in the case of the Moon, at greater distances.

Name Satellite of Difference in axes
km
% of mean
diameter
Mimas Saturn 33.4 (20.4 / 13.0) 8.4 (5.1 / 3.3)
Enceladus Saturn 16.6 3.3
Miranda Uranus 14.2 3.0
Tethys Saturn 25.8 2.4
Io Jupiter 29.4 0.8
Moon (Luna) Earth 4.3 0.1

Geological activity

Of the nineteen known natural satellites in the Solar System that are massive enough to have lapsed into hydrostatic equilibrium, several remain geologically active today. Io is the most volcanically active body in the Solar System, while Europa, Enceladus, Titan and Triton display evidence of ongoing tectonic activity and cryovolcanism. In the first three cases, the geological activity is powered by the tidal heating resulting from having eccentric orbits close to their giant-planet primaries. (This mechanism would have also operated on Triton in the past, before its orbit was circularized.) Many other natural satellites, such as Earth's Moon, Ganymede, Tethys and Miranda, show evidence of past geological activity, resulting from energy sources such as the decay of their primordial radioisotopes, greater past orbital eccentricities (due in some cases to past orbital resonances), or the differentiation or freezing of their interiors. Enceladus and Triton both have active features resembling geysers, although in the case of Triton solar heating appears to provide the energy. Titan and Triton have significant atmospheres; Titan also has hydrocarbon lakes, and presumably methane rain. Four of the largest natural satellites, Europa, Ganymede, Callisto, and Titan, are thought to have subsurface oceans of liquid water, while smaller Enceladus may have localized subsurface liquid water.

Natural satellites of the Solar System


Discovery image of Styx, photographed by Hubble’s Wide Field Camera 3[6]

The seven largest natural satellites in the Solar System (those bigger than 2,500 km across) are Jupiter's Galilean moons (Ganymede, Callisto, Io, and Europa), Saturn's moon Titan, Earth's moon, and Neptune's captured natural satellite Triton. Triton, the smallest of these, has more mass than all smaller natural satellites together. Similarly in the next size group of nine natural satellites, between 1,000 km and 1,600 km across, Titania, Oberon, Rhea, Iapetus, Charon, Ariel, Umbriel, Dione, and Tethys, the smallest, Tethys, has more mass than all smaller natural satellites together. As well as the natural satellites of the various planets, there are also over 80 known natural satellites of the dwarf planets, asteroids and other small Solar System bodies. Some studies estimate that up to 15% of all trans-Neptunian objects could have satellites.

The following is a comparative table classifying the natural satellites in the Solar System by diameter. The column on the right includes some notable planets, dwarf planets, asteroids, and trans-Neptunian objects for comparison. The natural satellites of the planets are named after mythological figures. These are predominately Greek, except for the Uranian natural satellites, which are named after Shakespearean characters. The nineteen bodies massive enough to have achieved hydrostatic equilibrium are in bold in the table below. Minor planets and satellites suspected but not proven to have achieved a hydrostatic equilibrium are italicized in the table below.

Mean
diameter
(km)
Satellites of planets Satellites of dwarf planets Satellites of
other
minor planets
Non-satellites
for comparison
Earth Mars Jupiter Saturn Uranus Neptune Pluto Haumea Eris
4,000–6,000 Ganymede
Callisto
Titan Mercury
3,000–4,000 Moon Io
Europa
2,000–3,000 Triton Eris
Pluto
1,000–2,000 Rhea
Iapetus
Dione
Tethys
Titania
Oberon
Umbriel
Ariel
Charon Makemake
Haumea
2007 OR10,
Quaoar
500–1,000 Enceladus Dysnomia 90377 Sedna, Ceres,
Salacia, Orcus,
2 Pallas4 Vesta
many more TNOs
250–500 Mimas
Hyperion
Miranda Proteus
Nereid
Hiʻiaka Orcus I Vanth 10 Hygiea
704 Interamnia
87 Sylvia
and many others
100–250 Amalthea
Himalia
Thebe
Phoebe
Janus
Epimetheus
Sycorax
Puck
Portia
Larissa
Galatea
Despina
Namaka S/2005 (82075) 1
Sila–Nunam I
Salacia I Actaea
Ceto I Phorcys
Patroclus I Menoetius
~21 more moons of TNOs
3 Juno
1992 QB1
5 Astraea
42355 Typhon
and many others
50–100 Elara
Pasiphae
Prometheus
Pandora
Caliban
Juliet
Belinda
Cressida
Rosalind
Desdemona
Bianca
Thalassa
Halimede
Neso
Naiad
Hydra
Nix
Quaoar I Weywot
90 Antiope I
Typhon I Echidna
Logos I Zoe
5 more moons of TNOs
90 Antiope
58534 Logos
253 Mathilde
and many others
25–50 Carme
Metis
Sinope
Lysithea
Ananke
Siarnaq
Helene
Albiorix
Atlas
Pan
Ophelia
Cordelia
Setebos
Prospero
Perdita
Stephano
Sao
Laomedeia
Psamathe
22 Kalliope I Linus 1036 Ganymed
243 Ida
and many others
10–25 Phobos
Deimos
Leda
Adrastea
Telesto
Paaliaq
Calypso
Ymir
Kiviuq
Tarvos
Ijiraq
Erriapus
Mab
Cupid
Francisco
Ferdinand
Margaret
Trinculo
S/2004 N 1 Kerberos
Styx
762 Pulcova I
Sylvia I Romulus
624 Hektor I
Eugenia I Petit-Prince
121 Hermione I
283 Emma I
1313 Berna I
107 Camilla I
433 Eros
1313 Berna
and many others
< 10 51 moons 36 moons Sylvia II Remus
Ida I Dactyl
and many others
many

Terminology


Montage comparing the relative sizes of selected natural satellites with the terrestrial planets and the dwarf planet Pluto

The first known natural satellite was the Moon, but it was considered a "planet" until Copernicus' introduction of heliocentrism in 1543. Until the discovery of the Galilean satellites in 1610, however, there was no opportunity for referring to such objects as a class. Galileo chose to refer to his discoveries as Planetæ ("planets"), but later discoverers chose other terms to distinguish them from the objects they orbited.

Christiaan Huygens, the discoverer of Titan, was the first to use the term moon for such objects, calling Titan Luna Saturni or Luna Saturnia – "Saturn's moon" or "The Saturnian moon", because it stood in the same relation to Saturn as the Moon did to Earth.[citation needed]

The first to use of the term satellite to describe orbiting bodies was the German astronomer Johannes Kepler in his pamphlet Narratio de Observatis a se quatuor Iouis satellitibus erronibus ("Narration About Four Satellites of Jupiter Observed") in 1610. He derived the term from the Latin word satelles, meaning "guard", "attendant", or "companion", because the satellites accompanied their primary planet in their journey through the heavens.

As additional natural satellites of Saturn were discovered the term "moon" was abandoned. Giovanni Domenico Cassini sometimes referred to his discoveries as planètes in French, but more often as satellites.[citation needed]

The term satellite thus became the normal one for referring to an object orbiting a planet, as it avoided the ambiguity of "moon". In 1957, however, the launching of the artificial object Sputnik created a need for new terminology. The terms man-made satellite or artificial moon were very quickly abandoned in favor of the simpler satellite, and as a consequence, the term has become linked primarily with artificial objects flown in space – including, sometimes, even those not in orbit around a planet.

Because of this shift in meaning, the term moon, which had continued to be used in a generic sense in works of popular science and in fiction, has regained respectability and is now used interchangeably with natural satellite, even in scientific articles. When it is necessary to avoid both the ambiguity of confusion with the Earth's natural satellite the Moon and the natural satellites of the other planets on the one hand, and artificial satellites on the other, the term natural satellite (using "natural" in a sense opposed to "artificial") is used. To further avoid ambiguity, the convention is to capitalize the word Moon when referring to the Earth's natural satellite, but not when referring to other natural satellites.

The definition of a moon


Comparison of Earth and the Moon

There is not an established lower limit on what is considered a "moon", as natural satellites will be referred to in this section. Every natural celestial body with an identified orbit around a planet of the Solar System, some as small as a kilometer across, has been identified as a moon, though objects a tenth that size within Saturn's rings, which have not been directly observed, have been called moonlets. Small asteroid moons (natural satellites of asteroids), such as Dactyl, have also been called moonlets.[14]

The upper limit is also vague. Two orbiting bodies are sometimes described as a double body rather than primary and satellite. Asteroids such as 90 Antiope are considered double asteroids, but they have not forced a clear definition of what constitutes a moon. Some authors consider the Pluto–Charon system to be a double (dwarf) planet. The most common[citation needed] dividing line on what is considered a moon rests upon whether the barycentre is below the surface of the larger body, though this is somewhat arbitrary, as it relies on distance as well as relative mass.

Visual summary

Solar System moons
Ganymede g1 true 2.jpg
Two Halves of Titan.png
Callisto.jpg
Io highest resolution true color.jpg
FullMoon2010.jpg
Europa-moon.jpg
Triton Voyager 2.jpg
Ganymede
(moon of Jupiter)
Titan
(moon of Saturn)
Callisto
(moon of Jupiter)
Io
(moon of Jupiter)
Moon
(moon of Earth)
Europa
(moon of Jupiter)
Triton
(moon of Neptune)
Titania (moon) color cropped.jpg
PIA07763 Rhea full globe5.jpg
Voyager 2 picture of Oberon.jpg
Iapetus as seen by the Cassini probe - 20071008.jpg
PIA00040 Umbrielx2.47.jpg
Ariel-NASA.jpg
Dione color south.jpg
Titania
(moon of Uranus)
Rhea
(moon of Saturn)
Oberon
(moon of Uranus)
Iapetus
(moon of Saturn)
Umbriel
(moon of Uranus)
Ariel
(moon of Uranus)
Dione
(moon of Saturn)
Inset-sat tethys-large.jpg
Enceladus from Voyager.jpg
Miranda.jpg
Proteus Voyager 2 cropped.jpg
Mimas PIA12569.jpg
Hyperion false color.jpg
Phoebe cassini.jpg
Tethys
(moon of Saturn)
Enceladus
(moon of Saturn)
Miranda
(moon of Uranus)
Proteus
(moon of Neptune)
Mimas
(moon of Saturn)
Hyperion
(moon of Saturn)
Phoebe
(moon of Saturn)
PIA12714 Janus crop.jpg
Amalthea (moon).png
PIA09813 Epimetheus S. polar region.jpg
Thebe.jpg
Prometheus 12-26-09a.jpg
Flying By Pandora.jpg
Leading hemisphere of Helene - 20110618.jpg
Janus
(moon of Saturn)
Amalthea
(moon of Jupiter)
Epimetheus
(moon of Saturn)
Thebe
(moon of Jupiter)
Prometheus
(moon of Saturn)
Pandora
(moon of Saturn)
Helene
(moon of Saturn)
Atlas (NASA).jpg
Telesto cassini closeup.jpg
N00151485 Calypso crop.jpg
Phobos colour 2008.jpg
Deimos-MRO.jpg
Methone PIA14633.jpg
Atlas
(moon of Saturn)
Telesto
(moon of Saturn)
Calypso
(moon of Saturn)
Phobos
(moon of Mars)
Deimos
(moon of Mars)
Methone
(moon of Saturn)


Introduction to entropy

From Wikipedia, the free encyclopedia https://en.wikipedia.org/wiki/Introduct...