Portal:Outer space
![]() | Portal maintenance status: (April 2019)
|
Introduction
![](http://webcf.waybackmachine.org/web/20220324124150im_/https://upload.wikimedia.org/wikipedia/commons/thumb/8/8c/Earth%27s_atmosphere.svg/300px-Earth%27s_atmosphere.svg.png)
Outer space, commonly shortened to space, is the expanse that exists beyond Earth and its atmosphere and between celestial bodies. Outer space is not completely empty—it is a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium, as well as electromagnetic radiation, magnetic fields, neutrinos, dust, and cosmic rays. The baseline temperature of outer space, as set by the background radiation from the Big Bang, is 2.7 kelvins (−270.45 °C; −454.81 °F). The plasma between galaxies is thought to account for about half of the baryonic (ordinary) matter in the universe, having a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvins. Local concentrations of matter have condensed into stars and galaxies. Studies indicate that 90% of the mass in most galaxies is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Observations suggest that the majority of the mass-energy in the observable universe is dark energy, a type of vacuum energy that is poorly understood. Intergalactic space takes up most of the volume of the universe, but even galaxies and star systems consist almost entirely of empty space.
Outer space does not begin at a definite altitude above the Earth's surface. The Kármán line, an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which entered into force on 10 October 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.
Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights. This was followed by crewed rocket flights and, then, crewed Earth orbit, first achieved by Yuri Gagarin of the Soviet Union in 1961. Due to the high cost of getting into space, human spaceflight has been limited to low Earth orbit and the Moon. On the other hand, uncrewed spacecraft have reached all of the known planets in the Solar System.
Outer space represents a challenging environment for human exploration because of the hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is very high. (Full article...)
Selected article
Halley's Comet is the best-known of the short-period comets, and is visible from Earth every 75 to 76 years. Halley is the only short-period comet that is clearly visible to the naked eye, and thus, the only naked-eye comet that might appear twice in a human lifetime. Other naked-eye comets may be brighter and more spectacular, but will appear only once in thousands of years. Halley's returns to the inner Solar System have been observed by astronomers since at least 240 BC, and recorded by Chinese, Babylonian, and mediaeval European chroniclers, but were not recognised as reappearances of the same object. The comet's periodicity was first determined in 1705 by English astronomer Edmond Halley, after whom it is now named. It last appeared in the inner Solar System in 1986 and will next appear in mid-2061. During its 1986 apparition, Halley's Comet became the first to be observed in detail by spacecraft, providing the first observational data on the structure of the comet nucleus and the mechanism of coma and tail formation. These observations supported a number of longstanding hypotheses about comet construction, particularly Fred Whipple's "dirty snowball" model, which correctly surmised that Halley would be composed of a mixture of volatile ices, such as water, carbon dioxide and ammonia, and dust. However, the missions also provided data which substantially reformed and reconfigured these ideas.
Selected picture
- Image 1The Sombrero Galaxy is a spiral galaxy in the Virgo constellation. It was discovered in the late 1700s. It is about 28 million light years away and is just faint enough to be invisible to the naked eye but easily visible with small telescopes. In our sky, it is about one-fifth the diameter of the full moon. M104 is moving away from Earth at about 1,000 kilometers per second.
- Image 2A timed exposure of the first Space Shuttle mission, STS-1. The shuttle Columbia stands on launch pad A at Kennedy Space Center, the night before launch. The objectives of the maiden flight were to check out the overall Shuttle system, accomplish a safe ascent into orbit and to return to Earth for a safe landing.
- Image 3A solar flare, a sudden flash of brightness observed over the Sun's surface or the solar limb which is interpreted as a large energy release, recorded on August 31, 2012. Such flares are often, but not always, followed by a colossal coronal mass ejection; in this instance, the ejection traveled at over 900 miles (1,400 km) per second.
- Image 4A composite photo of the Orion Nebula, the closest region of star formation to Earth. It is composed of 520 separate images and NASA calls it "one of the most detailed astronomical images ever produced". The nebula is located below Orion's Belt and is visible to the naked eye at night. It is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely-studied celestial features.
- Image 5A TRACE image of sunspots on the surface, or photosphere, of the sun from September 2002, is taken in the far ultraviolet on a relatively quiet day for solar activity. However, the image still shows a large sunspot group visible as a bright area near the horizon. Although sunspots are relatively cool regions on the surface of the sun, the bright glowing gas flowing around the sunspots have a temperature of over one million °C (1.8 million °F). The high temperatures are thought to be related to the rapidly changing magnetic field loops that channel solar plasma.
- Image 6Photo credit: Harrison SchmittAstronaut Eugene Cernan makes a short test drive of the lunar rover (officially, Lunar Roving Vehicle or LRV) during the early part of the first Apollo 17 extravehicular activity. The LRV was only used in the last three Apollo missions, but it performed without any major problems and allowed the astronauts to cover far more ground than in previous missions. All three LRVs were abandoned on the Moon.
- Image 7Credit: William Anders"Earthrise," the first occasion in which humans saw the Earth seemingly rising above the surface of the Moon, taken during the Apollo 8 mission on December 24, 1968. This view was seen by the crew at the beginning of its fourth orbit around the Moon, although the very first photograph taken was in black-and-white. Note that the Earth is in shadow here. A photo of a fully lit Earth would not be taken until the Apollo 17 mission.
- Image 8Photo: NASA/Crew of Expedition 22Space Shuttle Endeavour in a photograph taken from the International Space Station, in which the shuttle appears to straddle the stratosphere and mesosphere. During this mission, STS-130, the shuttle's primary payloads were the Tranquility module and the Cupola, a robotic control station which provides a 360-degree view around the station.
- Image 9Photograph credit: European Space AgencyMars is the fourth planet from the Sun and is known as the "Red Planet" due to its reddish appearance as seen from Earth. The planet is named after Mars, the Roman god of war. A terrestrial planet, Mars has a thin atmosphere and surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts and polar ice caps of the Earth. The planet has the highest mountain in the Solar System, Olympus Mons, as well as the largest canyon, Valles Marineris. Mars's rotation period and seasonal cycles are also similar to those of the Earth. Of all the planets in the Solar System other than Earth, Mars is the most likely to harbour liquid water and perhaps life. There are ongoing investigations assessing Mars's past potential for habitability, as well as the possibility of extant life. Future astrobiology missions are planned, including NASA's Mars 2020 rover and the European Space Agency (ESA)'s Rosalind Franklin rover. In November 2016, NASA reported finding a large amount of underground ice in the Utopia Planitia region of the planet. The volume of water detected has been estimated to be equivalent to the volume of water in Lake Superior. Mars has two moons, Phobos and Deimos, which are small and irregularly shaped.
This picture is a true-colour image of Mars, taken from a distance of about 240,000 kilometres (150,000 mi) by the OSIRIS instrument on ESA's Rosetta spacecraft, during its February 2007 flyby of the planet. The image was generated using OSIRIS's orange (red), green and blue filters. - Image 10Photo credit: Spirit roverA 360° panorama taken during the descent from the summit of Husband Hill, one of the Columbia Hills in Gusev crater, Mars. This stitched image is composed of 405 individual images taken with five different filters on the panoramic camera over the course of five Martian days.
- Image 11Photo: Yuri Beletsky, ESOA laser shoots towards the centre of the Milky Way from the Very Large Telescope facility in Chile, to provide a laser guide star, a reference point in the sky for the telescope's adaptive optics (AO) system. AO technology improves the performance of optical systems by reducing the effect of atmospheric distortion. AO was first envisioned by Horace W. Babcock in 1953, but did not come into common usage until advances in computer technology during the 1990s made the technique practical.
- Image 12Photo credit: NASAThe Eagle Nebula (also known as Messier Object 16, M16 or NGC 6611) is a young open cluster of stars. The nebula is an active region of star formation. Light from the bright, hot, young stars near the centre of the cluster illuminate the clouds of hydrogen gas and dust still collapsing to form new stars.
As projected on the sky, the Eagle Nebula lies in the constellation of Serpens Cauda. In three dimensions, it is relatively close to the Solar System being some 7,000 light years away on the edge of the Sagittarius Arm, the next nearest spiral arm towards the centre of the Milky Way.
In fact, when the picture is not coloured, is only red colored, the "Eagle" can be seen as a dark spot in the center of the nebula. - Image 13"The Blue Marble" is a famous photograph of Earth. NASA officially credits the image to the entire Apollo 17 crew — Eugene Cernan, Ronald Evans and Jack Schmitt — all of whom took photographic images during the mission. Apollo 17 passed over Africa during daylight hours and Antarctica is also illuminated. The photograph was taken approximately five hours after the spacecraft's launch, while en route to the Moon. Apollo 17, notably, was the last manned lunar mission; no humans since have been at a range where taking a "whole-Earth" photograph such as "The Blue Marble" would be possible.
- Image 14NGC 4414 is an unbarred spiral galaxy about 62 million light-years away in the constellation Coma Berenices. It is a flocculent spiral galaxy, with short segments of spiral structure but without the dramatic well-defined spiral arms of a grand design spiral. NGC 4414 is a very isolated galaxy, with no signs of past interactions with other galaxies.
- Image 15Credit: NASA, ESA, AURA/Caltech, Palomar ObservatoryThe Pleiades (also known as M45 or the Seven Sisters) is an open cluster in the constellation of Taurus. It is among the nearest to the Earth of all open clusters, probably the best known and certainly the most striking to the naked eye.
- Image 16Photograph credit: NASA / JPL / Space Science InstituteThe Cassini–Huygens space-research project involved a collaboration between NASA, the European Space Agency, and the Italian Space Agency to send a probe to study the planet Saturn and its system, including its rings and its natural satellites.
This natural-color mosaic image, combining thirty photographs, was taken by the Cassini orbiter over the course of approximately two hours on 23 July 2008 as it panned its wide-angle camera across Saturn and its ring system as the planet approached equinox. Six moons are pictured in the panorama, with the largest, Titan, visible at the bottom left. - Image 17Uranus is the seventh planet from the Sun and the fourth most massive in the Solar System. In this photograph from 1986 the planet appears almost featureless, but recent terrestrial observations have found seasonal changes to be occurring.
- Image 18Mercury is the smallest and closest to the Sun of the eight planets in the Solar System. It has no known natural satellites. The planet is named after the Roman deity Mercury, the messenger to the gods.
- Image 19Neptune is the eighth and farthest known planet from the Sun in the Solar System. In the Solar System, it is the fourth-largest planet by diameter, the third-most-massive planet and the densest giant planet. Neptune is 17 times the mass of Earth, slightly more massive than its near-twin Uranus. Neptune is denser and physically smaller than Uranus because its greater mass causes more gravitational compression of its atmosphere. Neptune orbits the Sun once every 164.8 years at an average distance of 30.1 au (4.5 billion km; 2.8 billion mi). It is named after the Roman god of the sea and has the astronomical symbol ♆, a stylised version of the god Neptune's trident.
This picture of Neptune was taken by NASA's Voyager 2 spacecraft in 1989, at a range of 4.4 million miles (7.1 million kilometres) from the planet, approximately four days before closest approach. The photograph shows the Great Dark Spot, a storm about the size of Earth, in the centre, while the fast-moving bright feature nicknamed the "Scooter" and the Small Dark Spot can be seen on the western limb. These clouds were seen to persist for as long as the spacecraft's cameras could resolve them. - Image 20Photo credit: Spitzer Space TelescopeThis infrared image shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because cosmic dust lying between Earth and the galactic center blocks our view.
- Image 21Image credit: Dave JarvisAn illustration of relative astronomical orders of magnitude, starting with the terrestrial planets of the Solar System in image 1 (top left) and ending with the largest known star, VY Canis Majoris, at the bottom right. The biggest celestial body in each image is shown on the left of the next frame.
- Image 22The Pioneer plaque, which was included on both Pioneer 10 and Pioneer 11 unmanned spacecraft, the first man-made objects to leave the Solar System. Made from gold-anodised aluminium, the plaque shows the figures of a man and a woman along with several symbols that are designed to provide information about the origin of the spacecraft. However, the mean time for the spacecraft to come within 30 astronomical units of a star is longer than the current age of our galaxy.
Space-related portals
Space news
- April 7: NASA's helicopter Ingenuity survives its first night at Mars
- December 25: 'Earth-based life can survive in hydrogen-rich atmospheres': MIT professor Dr Seager tells Wikinews about her research on organisms thriving in oxygen-less environment
- July 7: Astronomer Anthony Boccaletti discusses observation of birth of potential exoplanet with Wikinews
- May 31: SpaceX successfully launches its first crewed spaceflight
- May 22: Astronomer tells Wikinews about discovery of closest black hole known so far
- October 12: Cosmonaut Alexei Leonov dies at age 85
- October 10: Swedish academy announces 2019 Nobel Prize winners in physics
- September 14: Astronomers find water vapour in atmosphere of exoplanet K2-18b
- March 5: SpaceX Crew Dragon capsule docks with International Space Station
- January 9: Simple animals could live in Martian brines: Wikinews interviews planetary scientist Vlada Stamenković
- November 29: NASA's InSight Lander makes it to Mars
- October 12: Manned Soyuz space mission aborts during launch
2022 in space | |
---|---|
Space probe launches ![]() |
|
Impact events | |
Selected NEOs | |
Exoplanets ![]() |
|
Discoveries | |
Comets ![]() | |
Space exploration | |
Upcoming spaceflight launches
For a full launch schedule, see 2022 in spaceflight § Upcoming launches.
|
General images
Image 1Star cluster Pismis 24 and NGC 6357 (from Space exploration)
Image 2Matter distribution in a cubic section of the universe. The blue fiber structures represent the matter and the empty regions in between represent the cosmic voids of the intergalactic medium. (from Outer space)
Image 3The sparse plasma (blue) and dust (white) in the tail of comet Hale–Bopp are being shaped by pressure from solar radiation and the solar wind, respectively
Image 4A star-forming region in the Large Magellanic Cloud, perhaps the closest Galaxy to Earth's Milky Way (from Outer space)
Image 5Bow shock formed by the magnetosphere of the young star LL Orionis (center) as it collides with the Orion Nebula flow
Image 6The first image taken by a human of the whole Earth, probably photographed by William Anders of Apollo 8. South is up; South America is in the middle. (from Outer space)
Image 7Apollo 17 astronaut Harrison Schmitt standing next to a boulder at Taurus-Littrow. (from Space exploration)
Image 8Baker-Nunn cameras were widely used to study space debris. (from Space debris)
Image 9A view beneath the clouds of Titan, as seen in false colour, created from a mosaic of images taken by Cassini (2013) (from Space exploration)
Image 10This Kuiper belt object, known as Arrokoth, is the farthest closely visited Solar System body, seen in 2019 (from Space exploration)
Image 11Spatial density of LEO space debris by altitude, according to 2011 a NASA report to the United Nations Office for Outer Space Affairs (from Space debris)
Image 12A micrometeoroid left this crater on the surface of Space Shuttle Challenger's front window on STS-7. (from Space debris)
Image 13Three-dimensional structure in Pillars of Creation. (from Interstellar medium)
Image 14Triton as imaged by Voyager 2 (1989) (from Space exploration)
Image 15SpaceShipOne completed the first human private spaceflight in 2004, reaching an altitude of 100.12 km (62.21 mi).
Image 16Cosmic dust of the Andromeda Galaxy as revealed in infrared light by the Spitzer Space Telescope. (from Cosmic dust)
Image 17Aurora australis observed from the Space Shuttle Discovery, on STS-39, May 1991 (orbital altitude: 260 km)
Image 18Astronaut Piers Sellers during the third spacewalk of STS-121, a demonstration of orbiter heat shield repair techniques (from Outline of space science)
Image 19Crew quarters on Zvezda the base ISS crew module (from Space exploration)
Image 21Debris impacts on Mir's solar panels degraded their performance. The damage is most noticeable on the panel on the right, which is facing the camera with a high degree of contrast. Extensive damage to the smaller panel below is due to impact with a Progress spacecraft. (from Space debris)
Image 22Space Shuttle Endeavour had a major impact on its radiator during STS-118. The entry hole is about 5.5 mm (0.22 in), and the exit hole is twice as large. (from Space debris)
Image 23In July 1950 the first Bumper rocket is launched from Cape Canaveral, Florida. The Bumper was a two-stage rocket consisting of a Post-War V-2 topped by a WAC Corporal rocket. It could reach then-record altitudes of almost 400 km. Launched by General Electric Company, this Bumper was used primarily for testing rocket systems and for research on the upper atmosphere. They carried small payloads that allowed them to measure attributes including air temperature and cosmic ray impacts. (from Space exploration)
Image 24Sputnik 1, the first artificial satellite orbited Earth at 939 to 215 km (583 to 134 mi) in 1957, and was soon followed by Sputnik 2. See First satellite by country (Replica Pictured) (from Space exploration)
Image 25Comet 103P/Hartley (2010) (from Space exploration)
Image 26The original Magdeburg hemispheres (lower left) used to demonstrate Otto von Guericke's vacuum pump (right)
Image 27Lunar Gateway, one of the planned space stations for crewed cislunar travel in the 2020s (from Outer space)
Image 28Delta-v's in km/s for various orbital maneuvers (from Space exploration)
Image 29The Moon (2010) (from Space exploration)
Image 30A laser-guided observation of the Milky Way Galaxy at the Paranal Observatory in Chile in 2010 (from Outline of space science)
Image 31Artistic image of a rocket lifting from a Saturn moon (from Space exploration)
Image 32The Blue Marble Earth picture taken during Apollo 17 (1972) (from Space exploration)
Image 33A computer-generated image representing the locations, but not relative sizes, of space debris as could be seen from high Earth orbit. The two main debris fields are the ring of objects in geosynchronous Earth orbit (GEO) and the cloud of objects in low Earth orbit (LEO). (from Space debris)
Image 34Uranus as imaged by Voyager 2 (1986) (from Space exploration)
Image 35Cleanspace One (from Space debris)
Image 36Porous chondrite interplanetary dust particle. (from Cosmic dust)
Image 37Chandra, Hubble, and Spitzer image NGC 1952 (from Space exploration)
Image 38Map showing the Sun located near the edge of the Local Interstellar Cloud and Alpha Centauri about 4 light-years away in the neighboring G-Cloud complex (from Interstellar medium)
Image 39A picture of Neptune taken by Voyager 2 (1989) (from Space exploration)
Image 40Cosmic dust of the Horsehead Nebula as revealed by the Hubble Space Telescope. (from Cosmic dust)
Image 41A drifting thermal blanket photographed in 1998 during STS-88. (from Space debris)
Image 42Atmospheric attenuation in dB/km as a function of frequency over the EHF band. Peaks in absorption at specific frequencies are a problem, due to atmosphere constituents such as water vapor (H2O) and carbon dioxide (CO2). (from Interstellar medium)
Image 43Ganymede (moon) (from Space exploration)
Image 44The diversity found in the different types and scales of astronomical objects make the field of study increasingly specialized. (from Outline of space science)
Image 45Spatial density of space debris by altitude according to ESA MASTER-2001, without debris from the Chinese ASAT and 2009 collision events (from Space debris)
Image 46Asteroid 4 Vesta, imaged by the Dawn spacecraft (2011) (from Space exploration)
Image 47Reconstruction of solar activity over 11,400 years. Period of equally high activity over 8,000 years ago marked. (from Space climate)
Image 48This light-year-long knot of interstellar gas and dust resembles a caterpillar. (from Interstellar medium)
Image 49Artist's impression of dust formation around a supernova explosion. (from Cosmic dust)
Image 50Smooth chondrite interplanetary dust particle. (from Cosmic dust)
Image 51A MESSENGER image from 18,000 km showing a region about 500 km across (2008) (from Space exploration)
Image 52Most orbital flight actually takes place in upper layers of the atmosphere, especially in the thermosphere (not to scale) (from Space exploration)
Image 53Timeline of Solar System exploration. (from Space exploration)
Image 54Astronaut Buzz Aldrin had a personal Communion service when he first arrived on the surface of the Moon. (from Space exploration)
Image 55Spent upper stage of a Delta II rocket, photographed by the XSS 10 satellite (from Space debris)
Image 56The United States' planned Space Launch System concept art (from Space exploration)
Image 57Mars, as seen by the Hubble Space Telescope (2003) (from Space exploration)
Image 58Whirlpool Galaxy (Messier 51) (from Space exploration)
Image 59Herbig–Haro object HH 110 ejects gas through interstellar space. (from Interstellar medium)
Image 60Saudi officials inspect a crashed PAM-D module in January 2001. (from Space debris)
Image 61A dusty trail from the early Solar System to carbonaceous dust today. (from Cosmic dust)
Image 62The Long Duration Exposure Facility (LDEF) is an important source of information on small-particle space debris. (from Space debris)
Image 63Phobos (moon) (2008) (from Space exploration)
Image 64A picture of Saturn taken by Cassini (2004) (from Space exploration)
Image 65The interface between the Earth's surface and outer space. The Kármán line at an altitude of 100 km (62 mi) is shown. The layers of the atmosphere are drawn to scale, whereas objects within them, such as the International Space Station, are not. (from Outer space)
Image 66The Moon as seen in a digitally processed image from data collected during the 1992 Galileo spacecraft flyby (from Space exploration)
Image 67Opel RAK.1 - World's first public crewed flight of a rocket plane on September 30, 1929. (from Space exploration)
Image 682008 launch of the SM-3 missile used to destroy American reconnaissance satellite USA-193
Image 69Objects in Earth orbit including fragmentation debris. November 2020 NASA:ODPO (from Space debris)
Image 70New Horizons image of Charon (2015) (from Space exploration)
Image 71Mariner 10 image of Venus (1974) (from Space exploration)
Image 72Apollo CSM in lunar orbit (from Space exploration)
Image 73MESSENGER image of Mercury (2013) (from Space exploration)
Image 74Humans explore the lunar surface (from Space exploration)
Image 75The distribution of ionized hydrogen (known by astronomers as H II from old spectroscopic terminology) in the parts of the Galactic interstellar medium visible from the Earth's northern hemisphere as observed with the Wisconsin Hα Mapper (Haffner et al. 2003) harv error: no target: CITEREFHaffnerReynoldsTufteMadsen2003 (help). (from Interstellar medium)
Image 76Orbit of 2020 SO (from Space debris)
Image 77This is an artist's concept of the metric expansion of space, where a volume of the Universe is represented at each time interval by the circular sections. At left is depicted the rapid inflation from the initial state, followed thereafter by steadier expansion to the present day, shown at right. (from Outer space)
Image 78Space Shuttle Discovery's lower starboard wing and Thermal Protection System tiles, photographed on STS-114 during an R-Bar Pitch Manoeuvre where astronauts examine the TPS for any damage during ascent (from Space debris)
Image 79Concept art for a NASA Vision mission (from Space exploration)
Image 80Gabbard diagram of almost 300 pieces of debris from the disintegration of the five-month-old third stage of the Chinese Long March 4 booster on 11 March 2000 (from Space debris)
Image 81Voyager 1 is the first artificial object to reach the interstellar medium. (from Interstellar medium)
Image 82Major elements of 200 stratospheric interplanetary dust particles. (from Cosmic dust)
Image 83Surface of Mars by the Spirit rover (2004) (from Space exploration)
Image 84Vanguard 1 is expected to remain in orbit for 240 years. (from Space debris)
Image 85Apollo 16 LEM Orion, the Lunar Roving Vehicle and astronaut John Young (1972) (from Space exploration)
Image 86New Horizons image of Pluto (2015) (from Space exploration)
Image 87First television image of Earth from space, taken by TIROS-1. (1960) (from Space exploration)
Image 88Known orbit planes of Fengyun-1C debris one month after the weather satellite's disintegration by the Chinese ASAT (from Space debris)
Image 89A proposed timeline of the origin of space, from physical cosmology (from Outline of space science)
Image 90Zodiacal light caused by cosmic dust. (from Cosmic dust)
Image 91Part of the Hubble Ultra-Deep Field image showing a typical section of space containing galaxies interspersed by deep vacuum. Given the finite speed of light, this view covers the past 13 billion years of the history of outer space.
Image 92Because of the hazards of a vacuum, astronauts must wear a pressurized space suit while off-Earth and outside their spacecraft.
Astronomical events
Topics
Biology |
| |||||
---|---|---|---|---|---|---|
Technology |
| |||||
Society | ||||||
Environment | ||||||
2020 in space | ||
---|---|---|
Space probe launches ![]() |
| |
Impact events | ||
Selected NEOs |
| |
Exoplanets ![]() |
| |
Discoveries |
| |
Comets ![]() | ||
Space exploration |
| |
2019 in space | ||
---|---|---|
Space probe launches ![]() |
| |
Impact events |
| |
Selected NEOs | ||
Exoplanets ![]() |
| |
Discoveries |
| |
Comets ![]() | ||
Space exploration |
| |
2018 in space | ||
---|---|---|
Space probe launches ![]() |
| |
Impact events | ||
Selected NEOs | ||
Exoplanets ![]() | ||
Discoveries |
| |
Novae |
| |
Comets ![]() | ||
Space exploration |
| |
2017 in space | ||
---|---|---|
Space probe launches ![]() |
| |
Impact events | ||
Selected NEOs | ||
Exoplanets ![]() |
| |
Discoveries | ||
Comets ![]() | ||
Space exploration |
| |
2016 in space | ||
---|---|---|
Space probe launches ![]() |
| |
Impact events | ||
Selected NEOs | ||
Exoplanets ![]() |
| |
Discoveries |
| |
Novae | ||
Comets ![]() | ||
Space exploration | ||
2015 in space | ||||||
---|---|---|---|---|---|---|
Space probe launches ![]() |
| |||||
Impact events | ||||||
Selected NEOs | ||||||
Exoplanets ![]() |
| |||||
Discoveries |
| |||||
Comets ![]() | ||||||
Space exploration | ||||||
Categories
Wikimedia
The following Wikimedia Foundation sister projects provide more on this subject:
Wikibooks
Books
Commons
Media
Wikinews
News
Wikiquote
Quotations
Wikisource
Texts
Wikiversity
Learning resources
Wiktionary
Definitions
Wikidata
Database
Portals