From Wikipedia, the free encyclopedia
A
Bussard ramjet, one of many possible methods that could serve as propulsion of a starship.
Interstellar travel is the term used for hypothetical
crewed or uncrewed travel between
stars or
planetary systems. Interstellar travel will be much more difficult than
interplanetary spaceflight; the distances between the
planets in the
Solar System are less than 30
astronomical units (AU)—whereas the distances between stars are typically hundreds of thousands of AU, and usually expressed in
light-years. Because of the vastness of those distances, interstellar travel would require a high percentage of the
speed of light; huge travel time, lasting from decades to millennia or longer; or a combination of both.
The speeds required for interstellar travel in a human lifetime far exceed what current methods of
spacecraft propulsion can provide. Even with a hypothetically perfectly efficient propulsion system, the
kinetic energy corresponding to those speeds is enormous by today's standards of
energy production. Moreover, collisions by the spacecraft with
cosmic dust and gas can produce very dangerous effects both to passengers and the spacecraft itself.
A number of strategies have been proposed to deal with these
problems, ranging from giant arks that would carry entire societies and
ecosystems, to microscopic
space probes. Many different
spacecraft propulsion systems have been proposed to give spacecraft the required speeds, including
nuclear propulsion,
beam-powered propulsion, and methods based on speculative physics.
[1]
For both crewed and uncrewed interstellar travel, considerable
technological and economic challenges need to be met. Even the most
optimistic views about interstellar travel see it as only being feasible
decades from now—the more common view is that it is a century or more
away. However, in spite of the challenges, if interstellar travel should
ever be realized, then a wide range of scientific benefits can be
expected.
[2]
Most interstellar travel concepts require a developed space logistics
system capable of moving millions of tons to a construction / operating
location, and most would require gigawatt-scale power for construction
or power (such as
Star Wisp or
Light Sail type concepts). Such a system could grow organically if
space-based solar power
became a significant component of Earth's energy mix. Consumer demand
for a multi-terawatt system would automatically create the necessary
multi-million ton/year logistical system.
[3]
Challenges
Interstellar distances
Distances
between the planets in the Solar System are often measured in
astronomical units (AU), defined as the average distance between the Sun
and Earth, some 1.5
×10
8 kilometers (93 million miles).
Venus, the closest other planet to Earth is (at closest approach) 0.28 AU away.
Neptune, the farthest planet from the Sun, is 29.8 AU away. As of January 2018,
Voyager 1, the farthest man-made object from Earth, is 141.5 AU away.
[4]
The closest known star
Proxima Centauri, however, is some 268,332 AU away, or over 9,000 times farther away than Neptune.
Object |
A.U. |
light time |
Moon |
0.0026 |
1.3 seconds |
Sun |
1 |
8 minutes |
Venus (nearest planet) |
0.28 |
2.41 minutes |
Neptune (farthest planet) |
29.8 |
4.1 hours |
Voyager 1 |
141.5 |
19.61 hours |
Proxima Centauri (nearest star and exoplanet) |
268,332 |
4.24 years |
Because of this, distances between stars are usually expressed in
light-years, defined as the distance that a ray of
light travels in a year. Light in a vacuum travels around 300,000 kilometres (186,000 mi) per second, so this is some 9.461
×10
12 kilometers (5.879 trillion miles) or 1 light-year (63,241 AU) in a year. Proxima Centauri is 4.243 light-years away.
Another way of understanding the vastness of interstellar distances is by scaling: One of the closest stars to the Sun,
Alpha Centauri A (a Sun-like star), can be pictured by scaling down the
Earth–Sun distance to one meter (3.28 ft). On this scale, the distance to Alpha Centauri A would be 276 kilometers (171 miles).
The fastest outward-bound spacecraft yet sent,
Voyager 1,
has covered 1/600 of a light-year in 30 years and is currently moving
at 1/18,000 the speed of light. At this rate, a journey to Proxima
Centauri would take 80,000 years.
[5]
Required energy
A
significant factor contributing to the difficulty is the energy that
must be supplied to obtain a reasonable travel time. A lower bound for
the required energy is the
kinetic energy where
is the final mass. If
deceleration
on arrival is desired and cannot be achieved by any means other than
the engines of the ship, then the lower bound for the required energy is
doubled to
.
[6]
The velocity for a manned round trip of a few decades to even the
nearest star is several thousand times greater than those of present
space vehicles. This means that due to the
term in the kinetic energy formula, millions of times as much energy is
required. Accelerating one ton to one-tenth of the speed of light
requires at least 450 petajoules or 4.50
×10
17 joules or 125 terawatt-hours
[7] (
world energy consumption 2008 was 143,851 terawatt-hours),
[citation needed]
without factoring in efficiency of the propulsion mechanism. This
energy has to be generated onboard from stored fuel, harvested from the
interstellar medium, or projected over immense distances.
Interstellar medium
A knowledge of the properties of the
interstellar gas and dust through which the vehicle must pass is essential for the design of any interstellar space mission.
[8]
A major issue with traveling at extremely high speeds is that
interstellar dust may cause considerable damage to the craft, due to the
high relative speeds and large kinetic energies involved. Various
shielding methods to mitigate this problem have been proposed.
[9]
Larger objects (such as macroscopic dust grains) are far less common,
but would be much more destructive. The risks of impacting such objects,
and methods of mitigating these risks, have been discussed in the
literature, but many unknowns remain
[10] and, owing to the inhomogeneous distribution of interstellar matter around the Sun, will depend on direction travelled.
[8] Although a high density interstellar medium may cause difficulties for many interstellar travel concepts,
interstellar ramjets, and some proposed concepts for decelerating interstellar spacecraft, would actually benefit from a denser interstellar medium.
[8]
Hazards
The crew of an interstellar ship would face several significant hazards, including the psychological effects of long-term
isolation, the effects of exposure to
ionizing radiation, and the physiological effects of
weightlessness to the muscles, joints, bones, immune system, and eyes. There also exists the risk of impact by
micrometeoroids and other
space debris. These risks represent challenges that have yet to be overcome.
[11]
Wait calculation
It
has been argued that an interstellar mission that cannot be completed
within 50 years should not be started at all. Instead, assuming that a
civilization is still on an increasing curve of propulsion system
velocity and not yet having reached the limit, the resources should be
invested in designing a better propulsion system. This is because a slow
spacecraft would probably be passed by another mission sent later with
more advanced propulsion (the incessant obsolescence postulate).
[12]
On the other hand, Andrew Kennedy has shown that if one calculates the
journey time to a given destination as the rate of travel speed derived
from growth (even exponential growth) increases, there is a clear
minimum in the total time to that destination from now.
[13]
Voyages undertaken before the minimum will be overtaken by those who
leave at the minimum, whereas those who leave after the minimum will
never overtake those who left at the minimum.
Prime targets for interstellar travel
There are 59 known
stellar systems
within 40 light years of the Sun, containing 81 visible stars. The
following could be considered prime targets for interstellar missions:
[12]
System |
Distance (ly) |
Remarks |
Alpha Centauri |
4.3 |
Closest system. Three stars (G2, K1, M5). Component A is similar to the Sun (a G2 star). On August 24, 2016, the discovery of an Earth-size exoplanet (Proxima Centauri b) orbiting in the habitable zone of Proxima Centauri was announced. |
Barnard's Star |
6 |
Small, low-luminosity M5 red dwarf. Second closest to Solar System. |
Sirius |
8.7 |
Large, very bright A1 star with a white dwarf companion. |
Epsilon Eridani |
10.8 |
Single K2 star slightly smaller and colder than the Sun. It has two
asteroid belts, might have a giant and one much smaller planet,[14] and may possess a Solar-System-type planetary system. |
Tau Ceti |
11.8 |
Single G8 star
similar to the Sun. High probability of possessing a Solar-System-type
planetary system: current evidence shows 5 planets with potentially two
in the habitable zone. |
Wolf 1061 |
~14 |
Wolf 1061 c
is 4.3 times the size of Earth; it may have rocky terrain. It also sits
within the ‘Goldilocks’ zone where it might be possible for liquid
water to exist.[15] |
Gliese 581 planetary system |
20.3 |
Multiple planet system. The unconfirmed exoplanet Gliese 581g and the confirmed exoplanet Gliese 581d are in the star's habitable zone. |
Gliese 667C |
22 |
A system with at least six planets. A record-breaking three of these
planets are super-Earths lying in the zone around the star where liquid
water could exist, making them possible candidates for the presence of
life.[16] |
Vega |
25 |
A very young system possibly in the process of planetary formation.[17] |
TRAPPIST-1 |
39 |
A recently discovered system which boasts 7 Earth-like planets, some
of which may have liquid water. The discovery is a major advancement in
finding a habitable planet and in finding a planet that could support
life. |
Existing and near-term astronomical technology is capable of finding
planetary systems around these objects, increasing their potential for
exploration
Proposed methods
Slow, uncrewed probes
Slow interstellar missions based on current and near-future
propulsion technologies are associated with trip times starting from
about one hundred years to thousands of years. These missions consist of
sending a robotic probe to a nearby star for exploration, similar to
interplanetary probes such as used in the
Voyager program.
[18]
By taking along no crew, the cost and complexity of the mission is
significantly reduced although technology lifetime is still a
significant issue next to obtaining a reasonable speed of travel.
Proposed concepts include
Project Daedalus,
Project Icarus,
Project Dragonfly,
Project Longshot.,
[19] and more recently
Breakthrough Starshot.
[20]
Fast, uncrewed probes
Nanoprobes
Near-lightspeed
nano spacecraft might be possible within the near future built on
existing microchip technology with a newly developed nanoscale thruster.
Researchers at the
University of Michigan
are developing thrusters that use nanoparticles as propellant. Their
technology is called "nanoparticle field extraction thruster", or
nanoFET. These devices act like small particle accelerators shooting conductive nanoparticles out into space.
[21]
Michio Kaku,
a theoretical physicist, has suggested that clouds of "smart dust" be
sent to the stars, which may become possible with advances in
nanotechnology.
Kaku also notes that a large number of nanoprobes would need to be sent
due to the vulnerability of very small probes to be easily deflected by
magnetic fields, micrometeorites and other dangers to ensure the
chances that at least one nanoprobe will survive the journey and reach
the destination.
[22]
Given the light weight of these probes, it would take much less
energy to accelerate them. With onboard solar cells, they could
continually accelerate using solar power. One can envision a day when a
fleet of millions or even billions of these particles swarm to distant
stars at nearly the speed of light and relay signals back to Earth
through a vast interstellar communication network.
As a near-term solution, small, laser-propelled interstellar probes,
based on current CubeSat technology were proposed in the context of
Project Dragonfly.
[19]
Slow, manned missions
In
crewed missions, the duration of a slow interstellar journey presents a
major obstacle and existing concepts deal with this problem in
different ways.
[23] They can be distinguished by the "state" in which humans are transported on-board of the spacecraft.
Generation ships
A
generation ship (or
world ship) is a type of
interstellar ark
in which the crew that arrives at the destination is descended from
those who started the journey. Generation ships are not currently
feasible because of the difficulty of constructing a ship of the
enormous required scale and the great biological and sociological
problems that life aboard such a ship raises.
[24][25][26][27]
Suspended animation
Scientists and writers have postulated various techniques for
suspended animation. These include human
hibernation and
cryonic preservation. Although neither is currently practical, they offer the possibility of
sleeper ships in which the passengers lie inert for the long duration of the voyage.
[28]
Frozen embryos
A
robotic interstellar mission carrying some number of frozen early stage human
embryos is another theoretical possibility. This method of
space colonization requires, among other things, the development of an
artificial uterus, the prior detection of a habitable
terrestrial planet, and advances in the field of fully autonomous
mobile robots and educational robots that would replace human parents.
[29]
Island hopping through interstellar space
Interstellar space is not completely empty; it contains trillions of icy bodies ranging from small asteroids (
Oort cloud) to possible
rogue planets.
There may be ways to take advantage of these resources for a good part
of an interstellar trip, slowly hopping from body to body or setting up
waystations along the way.
[30]
Fast missions
If
a spaceship could average 10 percent of light speed (and decelerate at
the destination, for manned missions), this would be enough to reach
Proxima Centauri in forty years. Several propulsion concepts have been proposed
[31]
that might be eventually developed to accomplish this (see also the
section below on propulsion methods), but none of them are ready for
near-term (few decades) developments at acceptable cost.
Time dilation
Assuming faster-than-light travel is impossible, one might conclude
that a human can never make a round-trip farther from Earth than 20
light years if the traveler is active between the ages of 20 and 60. A
traveler would never be able to reach more than the very few star
systems that exist within the limit of 20 light years from Earth. This,
however, fails to take into account relativistic
time dilation.
[32]
Clocks aboard an interstellar ship would run slower than Earth clocks,
so if a ship's engines were capable of continuously generating around
1 g of acceleration (which is comfortable for humans), the ship could
reach almost anywhere in the galaxy and return to Earth within 40 years
ship-time (see diagram). Upon return, there would be a difference
between the time elapsed on the astronaut's ship and the time elapsed on
Earth.
For example, a spaceship could travel to a star 32 light-years away, initially accelerating at a constant 1.03g (i.e. 10.1 m/s
2)
for 1.32 years (ship time), then stopping its engines and coasting for
the next 17.3 years (ship time) at a constant speed, then decelerating
again for 1.32 ship-years, and coming to a stop at the destination.
After a short visit, the astronaut could return to Earth the same way.
After the full round-trip, the clocks on board the ship show that 40
years have passed, but according to those on Earth, the ship comes back
76 years after launch.
From the viewpoint of the astronaut, onboard clocks seem to be
running normally. The star ahead seems to be approaching at a speed of
0.87 light years per ship-year. The universe would appear contracted
along the direction of travel to half the size it had when the ship was
at rest; the distance between that star and the Sun would seem to be 16
light years as measured by the astronaut.
At higher speeds, the time on board will run even slower, so the astronaut could travel to the center of the
Milky Way
(30,000 light years from Earth) and back in 40 years ship-time. But the
speed according to Earth clocks will always be less than 1 light year
per Earth year, so, when back home, the astronaut will find that more
than 60 thousand years will have passed on Earth.
Constant acceleration
This plot shows a ship capable of 1-
g (10 m/s
2 or about 1.0 ly/y
2) "felt" or proper-acceleration
[33] can go far, except for the problem of accelerating on-board propellant.
Regardless of how it is achieved, a propulsion system that could
produce acceleration continuously from departure to arrival would be the
fastest method of travel. A constant acceleration journey is one where
the propulsion system accelerates the ship at a constant rate for the
first half of the journey, and then decelerates for the second half, so
that it arrives at the destination stationary relative to where it
began. If this were performed with an acceleration similar to that
experienced at the Earth's surface, it would have the added advantage of
producing artificial "gravity" for the crew. Supplying the energy
required, however, would be prohibitively expensive with current
technology.
[34]
From the perspective of a planetary observer, the ship will appear to
accelerate steadily at first, but then more gradually as it approaches
the speed of light (which it cannot exceed). It will undergo
hyperbolic motion.
[35]
The ship will be close to the speed of light after about a year of
accelerating and remain at that speed until it brakes for the end of the
journey.
From the perspective of an onboard observer, the crew will feel a
gravitational field
opposite the engine's acceleration, and the universe ahead will appear
to fall in that field, undergoing hyperbolic motion. As part of this,
distances between objects in the direction of the ship's motion will
gradually contract until the ship begins to decelerate, at which time an
onboard observer's experience of the gravitational field will be
reversed.
When the ship reaches its destination, if it were to exchange a
message with its origin planet, it would find that less time had elapsed
on board than had elapsed for the planetary observer, due to
time dilation and
length contraction.
The result is an impressively fast journey for the crew.
Propulsion
Rocket concepts
All rocket concepts are limited by the
rocket equation, which sets the characteristic velocity available as a function of exhaust velocity and mass ratio, the ratio of initial (
M0, including fuel) to final (
M1, fuel depleted) mass.
Very high
specific power, the ratio of thrust to total vehicle mass, is required to reach interstellar targets within sub-century time-frames.
[36] Some heat transfer is inevitable and a tremendous heating load must be adequately handled.
Thus, for interstellar rocket concepts of all technologies, a key
engineering problem (seldom explicitly discussed) is limiting the heat
transfer from the exhaust stream back into the vehicle.
[37]
Ion engine
A type of electric propulsion, spacecraft such as
Dawn use an
ion engine.
In an ion engine, electric power is used to create charged particles of
the propellant, usually the gas xenon, and accelerate them to extremely
high velocities. The exhaust velocity of conventional rockets is
limited by the chemical energy stored in the fuel’s molecular bonds,
which limits the thrust to about 5 km/s.
This gives them high power[clarification needed]
(for lift-off from Earth, for example) but limits the top speed. By
contrast, ion engines have low force, but the top speed in principle is
limited only by the electrical power available on the spacecraft and on
the gas ions being accelerated. The exhaust speed of the charged
particles range from 15 km/s to 35 km/s.
[38]
Nuclear fission powered
Fission-electric
Nuclear-electric
or plasma engines, operating for long periods at low thrust and powered
by fission reactors, have the potential to reach speeds much greater
than chemically powered vehicles or nuclear-thermal rockets. Such
vehicles probably have the potential to power Solar System exploration
with reasonable trip times within the current century. Because of their
low-thrust propulsion, they would be limited to off-planet, deep-space
operation.
Electrically powered spacecraft propulsion powered by a portable power-source, say a
nuclear reactor, producing only small accelerations, would take centuries to reach for example 15% of the
velocity of light, thus unsuitable for interstellar flight during a single human lifetime.
[39]
Fission-fragment
Fission-fragment rockets use
nuclear fission
to create high-speed jets of fission fragments, which are ejected at
speeds of up to 12,000 km/s (7,500 mi/s). With fission, the energy
output is approximately 0.1% of the total mass-energy of the reactor
fuel and limits the effective exhaust velocity to about 5% of the
velocity of light. For maximum velocity, the reaction mass should
optimally consist of fission products, the "ash" of the primary energy
source, so no extra reaction mass need be bookkept in the mass ratio.
Nuclear pulse
Modern Pulsed Fission Propulsion Concept.
Based on work in the late 1950s to the early 1960s, it has been technically possible to build spaceships with
nuclear pulse propulsion engines, i.e. driven by a series of nuclear explosions. This propulsion system contains the prospect of very high
specific impulse (space travel's equivalent of fuel economy) and high
specific power.
[40]
Project Orion team member
Freeman Dyson proposed in 1968 an interstellar spacecraft using nuclear pulse propulsion that used pure
deuterium fusion detonations with a very high fuel-
burnup fraction. He computed an exhaust velocity of 15,000 km/s and a 100,000-tonne space vehicle able to achieve a 20,000 km/s
delta-v allowing a flight-time to
Alpha Centauri of 130 years.
[41]
Later studies indicate that the top cruise velocity that can
theoretically be achieved by a Teller-Ulam thermonuclear unit powered
Orion starship, assuming no fuel is saved for slowing back down, is
about 8% to 10% of the speed of light (0.08-0.1c).
[42]
An atomic (fission) Orion can achieve perhaps 3%-5% of the speed of
light. A nuclear pulse drive starship powered by fusion-antimatter
catalyzed nuclear pulse propulsion units would be similarly in the 10%
range and pure matter-antimatter annihilation rockets would be
theoretically capable of obtaining a velocity between 50% to 80% of the
speed of light. In each case saving fuel for slowing down halves the
maximum speed. The concept of using a
magnetic sail
to decelerate the spacecraft as it approaches its destination has been
discussed as an alternative to using propellant, this would allow the
ship to travel near the maximum theoretical velocity.
[43] Alternative designs utilizing similar principles include
Project Longshot,
Project Daedalus, and
Mini-Mag Orion. The principle of external nuclear pulse propulsion to maximize
survivable power has remained common among serious concepts for
interstellar flight without external power beaming and for very
high-performance interplanetary flight.
In the 1970s the Nuclear Pulse Propulsion concept further was refined by
Project Daedalus by use of externally triggered
inertial confinement fusion, in this case producing fusion explosions via compressing fusion fuel pellets with high-powered electron beams. Since then,
lasers,
ion beams,
neutral particle beams and hyper-kinetic projectiles have been suggested to produce nuclear pulses for propulsion purposes.
[44]
A current impediment to the development of
any nuclear-explosion-powered spacecraft is the
1963 Partial Test Ban Treaty,
which includes a prohibition on the detonation of any nuclear devices
(even non-weapon based) in outer space. This treaty would, therefore,
need to be renegotiated, although a project on the scale of an
interstellar mission using currently foreseeable technology would
probably require international cooperation on at least the scale of the
International Space Station.
Nuclear fusion rockets
Daedalus interstellar vehicle.
Fusion rocket starships, powered by
nuclear fusion
reactions, should conceivably be able to reach speeds of the order of
10% of that of light, based on energy considerations alone. In theory, a
large number of stages could push a vehicle arbitrarily close to the
speed of light.
[45] These would "burn" such light element fuels as deuterium, tritium,
3He,
11B, and
7Li.
Because fusion yields about 0.3–0.9% of the mass of the nuclear fuel as
released energy, it is energetically more favorable than fission, which
releases less than 0.1% of the fuel's mass-energy. The maximum exhaust
velocities potentially energetically available are correspondingly
higher than for fission, typically 4–10% of c. However, the most easily
achievable fusion reactions release a large fraction of their energy as
high-energy neutrons, which are a significant source of energy loss.
Thus, although these concepts seem to offer the best (nearest-term)
prospects for travel to the nearest stars within a (long) human
lifetime, they still involve massive technological and engineering
difficulties, which may turn out to be intractable for decades or
centuries.
Early studies include
Project Daedalus, performed by the
British Interplanetary Society in 1973–1978, and
Project Longshot, a student project sponsored by
NASA and the
US Naval Academy, completed in 1988. Another fairly detailed vehicle system, "Discovery II",
[46] designed and optimized for crewed Solar System exploration, based on the D
3He reaction but using hydrogen as reaction mass, has been described by a team from NASA's
Glenn Research Center. It achieves characteristic velocities of greater than 300 km/s with an acceleration of ~1.7•10
−3 g,
with a ship initial mass of ~1700 metric tons, and payload fraction
above 10%. Although these are still far short of the requirements for
interstellar travel on human timescales, the study seems to represent a
reasonable benchmark towards what may be approachable within several
decades, which is not impossibly beyond the current state-of-the-art.
Based on the concept's 2.2%
burnup fraction it could achieve a pure fusion product exhaust velocity of ~3,000 km/s.
Antimatter rockets
An
antimatter rocket would have a far higher energy density and specific impulse than any other proposed class of rocket.
[31] If energy resources and efficient production methods are found to make
antimatter in the quantities required and store
[47][48] it safely, it would be theoretically possible to reach speeds of several tens of percent that of light.
[31] Whether antimatter propulsion could lead to the higher speeds (>90% that of light) at which relativistic
time dilation
would become more noticeable, thus making time pass at a slower rate
for the travelers as perceived by an outside observer, is doubtful owing
to the large quantity of antimatter that would be required.
[31]
Speculating that production and storage of antimatter should become
feasible, two further issues need to be considered. First, in the
annihilation of antimatter, much of the energy is lost as high-energy
gamma radiation, and especially also as
neutrinos, so that only about 40% of
mc2 would actually be available if the antimatter were simply allowed to annihilate into radiations thermally.
[31] Even so, the energy available for propulsion would be substantially higher than the ~1% of
mc2 yield of nuclear fusion, the next-best rival candidate.
Second, heat transfer from the exhaust to the vehicle seems likely to
transfer enormous wasted energy into the ship (e.g. for 0.1
g
ship acceleration, approaching 0.3 trillion watts per ton of ship mass),
considering the large fraction of the energy that goes into penetrating
gamma rays. Even assuming shielding was provided to protect the payload
(and passengers on a crewed vehicle), some of the energy would
inevitably heat the vehicle, and may thereby prove a limiting factor if
useful accelerations are to be achieved.
More recently,
Friedwardt Winterberg
proposed that a matter-antimatter GeV gamma ray laser photon rocket is
possible by a relativistic proton-antiproton pinch discharge, where the
recoil from the laser beam is transmitted by the
Mössbauer effect to the spacecraft.
[49]
Rockets with an external energy source
Rockets deriving their power from external sources, such as a
laser,
could replace their internal energy source with an energy collector,
potentially reducing the mass of the ship greatly and allowing much
higher travel speeds.
Geoffrey A. Landis has proposed for an
interstellar probe, with energy supplied by an external laser from a base station powering an
Ion thruster.
[50]
Non-rocket concepts
A
problem with all traditional rocket propulsion methods is that the
spacecraft would need to carry its fuel with it, thus making it very
massive, in accordance with the
rocket equation. Several concepts attempt to escape from this problem:
[31][51]
Interstellar ramjets
In 1960,
Robert W. Bussard proposed the
Bussard ramjet, a fusion rocket in which a huge scoop would collect the diffuse hydrogen in interstellar space, "burn" it on the fly using a
proton–proton chain reaction,
and expel it out of the back. Later calculations with more accurate
estimates suggest that the thrust generated would be less than the drag
caused by any conceivable scoop design.
[citation needed] Yet the idea is attractive because the fuel would be collected
en route (commensurate with the concept of
energy harvesting),
so the craft could theoretically accelerate to near the speed of light.
The limitation is due to the fact that the reaction can only accelerate
the propellant to 0.12c. Thus the drag of catching interstellar dust
and the thrust of accelerating that same dust to 0.12c would be the same
when the speed is 0.12c, preventing further acceleration.
Beamed propulsion
A
light sail or
magnetic sail powered by a massive
laser
or particle accelerator in the home star system could potentially reach
even greater speeds than rocket- or pulse propulsion methods, because
it would not need to carry its own
reaction mass and therefore would only need to accelerate the craft's
payload.
Robert L. Forward
proposed a means for decelerating an interstellar light sail in the
destination star system without requiring a laser array to be present in
that system. In this scheme, a smaller secondary sail is deployed to
the rear of the spacecraft, whereas the large primary sail is detached
from the craft to keep moving forward on its own. Light is reflected
from the large primary sail to the secondary sail, which is used to
decelerate the secondary sail and the spacecraft payload.
[52] In 2002,
Geoffrey A. Landis of
NASA's
Glen Research center also proposed a laser-powered, propulsion, sail
ship that would host a diamond sail (of a few nanometers thick) powered
with the use of
solar energy.
[53] With this proposal, this interstellar ship would, theoretically, be able to reach 10 percent the speed of light.
A
magnetic sail
could also decelerate at its destination without depending on carried
fuel or a driving beam in the destination system, by interacting with
the plasma found in the solar wind of the destination star and the
interstellar medium.
[54][55]
The following table lists some example concepts using beamed laser propulsion as proposed by the physicist
Robert L. Forward:
[56]
Mission |
Laser Power |
Vehicle Mass |
Acceleration |
Sail Diameter |
Maximum Velocity (% of the speed of light) |
1. Flyby – Alpha Centauri, 40 years |
outbound stage |
65 GW |
1 t |
0.036 g |
3.6 km |
11% @ 0.17 ly |
2. Rendezvous – Alpha Centauri, 41 years |
outbound stage |
7,200 GW |
785 t |
0.005 g |
100 km |
21% @ 4.29 ly[dubious – discuss] |
deceleration stage |
26,000 GW |
71 t |
0.2 g |
30 km |
21% @ 4.29 ly |
3. Manned – Epsilon Eridani, 51 years (including 5 years exploring star system) |
outbound stage |
75,000,000 GW |
78,500 t |
0.3 g |
1000 km |
50% @ 0.4 ly |
deceleration stage |
21,500,000 GW |
7,850 t |
0.3 g |
320 km |
50% @ 10.4 ly |
return stage |
710,000 GW |
785 t |
0.3 g |
100 km |
50% @ 10.4 ly |
deceleration stage |
60,000 GW |
785 t |
0.3 g |
100 km |
50% @ 0.4 ly |
Interstellar travel catalog to use photogravitational assists for a full stop
The following table is based on work by Heller, Hippke and Kervella.
[57]
Name |
Travel time
(yr) |
Distance
(ly) |
Luminosity
(L☉) |
Sirius A |
68.90 |
8.58 |
24.20 |
α Centauri A |
101.25 |
4.36 |
1.52 |
α Centauri B |
147.58 |
4.36 |
0.50 |
Procyon A |
154.06 |
11.44 |
6.94 |
Vega |
167.39 |
25.02 |
50.05 |
Altair |
176.67 |
16.69 |
10.70 |
Fomalhaut A |
221.33 |
25.13 |
16.67 |
Denebola |
325.56 |
35.78 |
14.66 |
Castor A |
341.35 |
50.98 |
49.85 |
Epsilon Eridiani |
363.35 |
10.50 |
0.50 |
- Successive assists at α Cen A and B could allow travel times to 75 yr to both stars.
- Lightsail has a nominal mass-to-surface ratio (σnom) of 8.6×10−4 gram m−2 for a nominal graphene-class sail.
- Area of the Lightsail, about 105 m2 = (316 m)2
- Velocity up to 37,300 km s−1 (12.5% c)
Pre-accelerated fuel
Achieving
start-stop interstellar trip times of less than a human lifetime
require mass-ratios of between 1,000 and 1,000,000, even for the nearer
stars. This could be achieved by multi-staged vehicles on a vast scale.
[45] Alternatively large linear accelerators could propel fuel to fission propelled space-vehicles, avoiding the limitations of the
Rocket equation.
[58]
Theoretical concepts
Faster-than-light travel
Artist's depiction of a hypothetical
Wormhole Induction Propelled Spacecraft, based loosely on the 1994
"warp drive" paper of
Miguel Alcubierre. Credit: NASA CD-98-76634 by Les Bossinas.
Scientists and authors have postulated a number of ways by which it
might be possible to surpass the speed of light, but even the most
serious-minded of these are highly speculative.
[59]
It is also debatable whether faster-than-light travel is physically possible, in part because of
causality concerns: travel faster than light may, under certain conditions, permit travel backwards in time within the context of
special relativity.
[60] Proposed mechanisms for
faster-than-light travel within the theory of general relativity require the existence of
exotic matter[59] and it is not known if this could be produced in sufficient quantity.
Alcubierre drive
In physics, the
Alcubierre drive is based on an argument, within the framework of
general relativity and without the introduction of
wormholes,
that it is possible to modify a spacetime in a way that allows a
spaceship to travel with an arbitrarily large speed by a local expansion
of spacetime behind the spaceship and an opposite contraction in front
of it.
[61] Nevertheless, this concept would require the spaceship to incorporate a region of
exotic matter, or hypothetical concept of
negative mass.
[61]
Artificial black hole
A theoretical idea for enabling interstellar travel is by propelling a
starship by creating an artificial black hole and using a parabolic
reflector to reflect its Hawking radiation. Although beyond current
technological capabilities, a black hole starship offers some advantages
compared to other possible methods. Getting the black hole to act as a
power source and engine also requires a way to convert the Hawking
radiation into energy and thrust. One potential method involves placing
the hole at the focal point of a parabolic reflector attached to the
ship, creating forward thrust. A slightly easier, but less efficient
method would involve simply absorbing all the gamma radiation heading
towards the fore of the ship to push it onwards, and let the rest shoot
out the back.
[62][63][64]
Wormholes
Wormholes
are conjectural distortions in spacetime that theorists postulate could
connect two arbitrary points in the universe, across an
Einstein–Rosen Bridge.
It is not known whether wormholes are possible in practice. Although
there are solutions to the Einstein equation of general relativity that
allow for wormholes, all of the currently known solutions involve some
assumption, for example the existence of
negative mass, which may be unphysical.
[65] However, Cramer
et al. argue that such wormholes might have been created in the early universe, stabilized by
cosmic string.
[66] The general theory of wormholes is discussed by Visser in the book
Lorentzian Wormholes.
[67]
Hyperdrive
If the conjecture of Felber is correct, ie any mass moving at 57.7% C generates an
anti-gravity beam then an Orion drive may be capable of acting as the initial boost, and as-yet-undiscovered technology based on theorized
anti-matter repulsion effects under exotic conditions such as
entanglement that directly manipulates space-time to open a window into
hyperspace.
This could feasibly exploit physics in extradimensional space to travel
very quickly through the galaxy. The side effect here is that due to
the need for a second vehicle to slow down it would be a one-way trip,
although other concepts such as a solar sail could be used to slow down
near the destination.
[68] All the components could be feasibly re-used and also provide very effective
SETI
targets if other species are using this technology. It is also likely
that hyperdrive jumps could be limited to discrete areas such as near
stars due to gravitation wells.
Designs and studies
Enzmann starship
The Enzmann starship, as detailed by
G. Harry Stine in the October 1973 issue of
Analog, was a design for a future
starship, based on the ideas of Robert Duncan-Enzmann. The spacecraft itself as proposed used a 12,000,000 ton ball of frozen
deuterium to power 12–24 thermonuclear pulse propulsion units. Twice as long as the
Empire State Building and assembled in-orbit, the spacecraft was part of a larger project preceded by
interstellar probes and telescopic observation of target star systems.
[69]
Project Hyperion
Project Hyperion, one of the projects of
Icarus Interstellar.
[70]
NASA research
NASA
has been researching interstellar travel since its formation,
translating important foreign language papers and conducting early
studies on applying fusion propulsion, in the 1960s, and laser
propulsion, in the 1970s, to interstellar travel.
The
NASA Breakthrough Propulsion Physics Program (terminated in FY 2003 after a 6-year, $1.2-million study, because "No breakthroughs appear imminent.")
[71] identified some breakthroughs that are needed for interstellar travel to be possible.
[72]
Geoffrey A. Landis of NASA's
Glenn Research Center
states that a laser-powered interstellar sail ship could possibly be
launched within 50 years, using new methods of space travel. "I think
that ultimately we're going to do it, it's just a question of when and
who," Landis said in an interview. Rockets are too slow to send humans
on interstellar missions. Instead, he envisions interstellar craft with
extensive sails, propelled by laser light to about one-tenth the speed
of light. It would take such a ship about 43 years to reach Alpha
Centauri if it passed through the system. Slowing down to stop at Alpha
Centauri could increase the trip to 100 years,
[73]
whereas a journey without slowing down raises the issue of making
sufficiently accurate and useful observations and measurements during a
fly-by.
100 Year Starship study
The
100 Year Starship
(100YSS) is the name of the overall effort that will, over the next
century, work toward achieving interstellar travel. The effort will also
go by the moniker 100YSS. The 100 Year Starship study is the name of a
one-year project to assess the attributes of and lay the groundwork for
an organization that can carry forward the 100 Year Starship vision.
Harold ("Sonny") White[74] from NASA's Johnson Space Center is a member of
Icarus Interstellar,
[75]
the nonprofit foundation whose mission is to realize interstellar
flight before the year 2100. At the 2012 meeting of 100YSS, he reported
using a
laser to try to warp spacetime by 1 part in 10 million with the aim of helping to make interstellar travel possible.
[76]
Other designs
- Project Orion, manned interstellar ship (1958–1968).
- Project Daedalus, unmanned interstellar probe (1973–1978).
- Starwisp, unmanned interstellar probe (1985).[77]
- Project Longshot, unmanned interstellar probe (1987–1988).
- Starseed/launcher, fleet of unmanned interstellar probes (1996)
- Project Valkyrie, manned interstellar ship (2009)
- Project Icarus, unmanned interstellar probe (2009–2014).
- Sun-diver, unmanned interstellar probe[78]
- Breakthrough Starshot, fleet of unmanned interstellar probes, announced in April 12, 2016.[79][80][81]
Non-profit organizations
A
few organisations dedicated to interstellar propulsion research and
advocacy for the case exist worldwide. These are still in their infancy,
but are already backed up by a membership of a wide variety of
scientists, students and professionals.
Feasibility
The
energy requirements make interstellar travel very difficult. It has
been reported that at the 2008 Joint Propulsion Conference, multiple
experts opined that it was improbable that humans would ever explore
beyond the Solar System.
[87]
Brice N. Cassenti, an associate professor with the Department of
Engineering and Science at Rensselaer Polytechnic Institute, stated that
at least 100 times the total energy output of the entire world [in a
given year] would be required to send a probe to the nearest star.
[87]
Astrophysicist Sten Odenwald stated that the basic problem is that
through intensive studies of thousands of detected exoplanets, most of
the closest destinations within 50 light years do not yield Earth-like
planets in the star's habitable zones.
[88]
Given the multi-trillion-dollar expense of some of the proposed
technologies, travelers will have to spend up to 200 years traveling at
20% the speed of light to reach the best known destinations. Moreover,
once the travelers arrive at their destination (by any means), they will
not be able to travel down to the surface of the target world and set
up a colony unless the atmosphere is non-lethal. The prospect of making
such a journey, only to spend the rest of the colony's life inside a
sealed habitat and venturing outside in a spacesuit, may eliminate many
prospective targets from the list.
Moving at a speed close to the speed of light and encountering even a
tiny stationary object like a grain of sand will have fatal
consequences. For example, a gram of matter moving at 90% of the speed
of light contains a kinetic energy corresponding to a small nuclear bomb
(around 30kt TNT).
Interstellar missions not for human benefit
Explorative high-speed missions to
Alpha Centauri, as planned for by the
Breakthrough Starshot initiative, are projected to be realizable within the
21st century.
[89]
It is alternatively possible to plan for unmanned slow-cruising
missions taking millennia to arrive. These probes would not be for human
benefit in the sense that one can not foresee whether there would be
anybody around on earth interested in then back-transmitted science
data. An example would be the Genesis mission,
[90] which aims to bring unicellular life, in the spirit of
directed panspermia, to habitable but otherwise barren planets.
[91] Comparatively slow cruising Genesis probes, with a typical speed of
, corresponding to about
, can be decelerated using a
magnetic sail. Unmanned missions not for human benefit would hence be feasible
[92]
Discovery of Earth-Like planets
In
February 2017, NASA has announced the discovery of 7 Earth-like planets
in the TRAPPIST-1 system orbiting an ultra-cool dwarf star 40
light-years away from our solar system.
[93]
NASA's Spitzer Space Telescope has revealed the first known system of
seven Earth-size planets around a single star. Three of these planets
are firmly located in the habitable zone, the area around the parent
star where a rocky planet is most likely to have liquid water. The
discovery sets a new record for greatest number of habitable-zone
planets found around a single star outside our solar system. All of
these seven planets could have liquid water – the key to life as we know
it – under the right atmospheric conditions, but the chances are
highest with the three in the habitable zone.