Space research

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Short description: Scientific studies carried out using scientific equipment in outer space
One extent of space research is seen in the Opportunity mission
The first major scientific discovery made from space was the dangerous Van Allen radiation belts

Space research is scientific study carried out in outer space, and by studying outer space. From the use of space technology to the observable universe, space research is a wide research field. Earth science, materials science, biology, medicine, and physics all apply to the space research environment. The term includes scientific payloads at any altitude from deep space to low Earth orbit, extended to include sounding rocket research in the upper atmosphere, and high-altitude balloons.

Space exploration is also a form of space research.

History

The first US satellite was the Explorer 1, seen here launching, 1 February 1958
First image of the far side of the Moon, sent back to Earth by the Luna 3 mission

Rockets

China rockets were used in ceremony and as weaponry since the 13th century, but no rocket would overcome Earth's gravity until the latter half of the 20th century. Space-capable rocketry appeared simultaneously in the work of three scientists, in three separate countries. In Russia, Konstantin Tsiolkovsky, in the United States, Robert H. Goddard, and in Germany, Hermann Oberth.

The United States and the Soviet Union created their own missile programs. The space research field evolved as scientific investigation based on advancing rocket technology.

In 1948–1949 detectors on V-2 rocket flights detected x-rays from the Sun.[1] Sounding rockets helped show us the structure of the upper atmosphere. As higher altitudes were reached, space physics emerged as a field of research with studies of Earths aurorae, ionosphere and magnetosphere.

Artificial satellites

The first artificial satellite, Russian Sputnik 1, launched on October 4, 1957, four months before the United States first, Explorer 1. The major discovery of satellite research was in 1958, when Explorer 1 detected the Van Allen radiation belts. Planetology reached a new stage with the Russian Luna programme, between 1959 and 1976, a series of lunar probes which gave us evidence of the Moons chemical composition, gravity, temperature, soil samples, the first photographs of the far side of the Moon by Luna 3, and the first remotely controlled robots (Lunokhod) to land on another planetary body.

Yuri Gagarin was the first human being to travel in space

International co-operation

The early space researchers obtained an important international forum with the establishment of the Committee on Space Research (COSPAR) in 1958, which achieved an exchange of scientific information between east and west during the cold war, despite the military origin of the rocket technology underlying the research field.[2]

Astronauts

On April 12, 1961, Russian Lieutenant Yuri Gagarin was the first human to orbit Earth, in Vostok 1. In 1961, US astronaut Alan Shepard was the first American in space. And on July 20, 1969, astronaut Neil Armstrong was the first human on the Moon.

On April 19, 1971, the Soviet Union launched the Salyut 1, the first space station of substantial duration, a successful 23 day mission, sadly ruined by transport disasters. On May 14, 1973, Skylab, the first American space station launched, on a modified Saturn V rocket. Skylab was occupied for 24 weeks.[3]

Extent

486958 Arrokoth is the farthest object visited by human spacecraft

486958 Arrokoth is the name of the farthest and most primitive object visited by human spacecraft. Originally designated "1110113Y" when detected by Hubble in 2014, the planetessimal was reached by the New Horizons probe on 1 January 2019 after a week long manoeuvering phase. New Horizons detected Ultima Thule from 107 million miles and performed a total 9 days of manoeuvres to pass within 3,500 miles of the 19 mile long contact binary. Ultima Thule has an orbital period around 298 years, is 4.1 billion miles from Earth, and over 1 billion miles beyond Pluto.

Interstellar

The Voyager 1 probe launched on 5 September 1977, and flew beyond the edge of our solar system in August 2012 to the interstellar medium. The farthest human object from the Earth, predictions include collision, an Oort cloud, and destiny, "perhaps eternally—to wander the Milky Way."

Voyager 2 launched on 20 August 1977 travelling slower than Voyager 1 and reached interstellar medium by the end of 2018. Voyager 2 is the only Earth probe to have visited the ice giants of Neptune or Uranus

Neither Voyager is aimed at a particular visible object, but both continue to send research data to NASA Deep Space Network as of 2019.

Two Pioneer probes and the New Horizons probe are expected to enter interstellar medium in the near future, but these three are expected to have depleted available power before then, so the point of exit cannot be confirmed precisely. Predicting probes speed is imprecise as they pass through the variable heliosphere. Pioneer 10 is roughly at the outer edge of the heliosphere in 2019. New Horizons should reach it by 2040, and Pioneer 11 by 2060.

Two Voyager probes have reached interstellar medium, and three other probes are expected to join that list.

Research fields

Space research includes the following fields of science:[4][5]

Space research from artificial satellites

Upper Atmosphere Research Satellite

Upper Atmosphere Research Satellite was a NASA-led mission launched on September 12, 1991. The 5,900 kg (13,000 lb) satellite was deployed from the Space Shuttle Discovery during the STS-48 mission on 15 September 1991. It was the first multi-instrumented satellite to study various aspects of the Earth's atmosphere and have a better understanding of photochemistry. After 14 years of service, the UARS finished its scientific career in 2005.[6]

Great Observatories program

Great Observatories program telescopes are combined for enhanced detail in this image of the Crab Nebula

Great Observatories program is the flagship NASA telescope program. The Great Observatories program pushes forward our understanding of the universe with detailed observation of the sky, based in gamma rays, ultraviolet, x-ray, infrared, and visible, light spectrums. The four main telescopes for the Great Observatories program are, Hubble Space Telescope (visible, ultraviolet), launched 1990, Compton Gamma Ray Observatory (gamma), launched 1991 and retired 2000, Chandra X-Ray Observatory (x-ray), launched 1999, and Spitzer Space Telescope (infrared), launched 2003.

Origins of the Hubble, named after American astronomer Edwin Hubble, go back as far as 1946. In the present day, the Hubble is used to identify exo-planets and give detailed accounts of events in our own solar system. Hubbles visible-light observations are combined with the other great observatories to give us some of the most detailed images of the visible universe.

International Gamma-Ray Astrophysics Laboratory

INTEGRAL is one of the most powerful gamma-ray observatories, launched by the European Space Agency in 2002, and continuing to operate (as of March 2019). INTEGRAL provides insight into the most energetic cosmological formations in space including, black holes, neutron stars, and supernovas.[7] INTEGRAL plays an important role researching gamma-rays, one of the most exotic and energetic phenomena in space.

Gravity and Extreme Magnetism Small Explorer

The NASA-led GEMS mission was scheduled to launch for November 2014.[8] The spacecraft would use an X-Ray telescope to measure the polarization of x-rays coming from black holes and neutron stars. It would research into remnants of supernovae, stars that have exploded. Few experiments have been conducted in X-Ray polarization since the 1970s, and scientists anticipated GEMS to break new ground. Understanding x-ray polarisation will improve scientists knowledge of black holes, in particular whether matter around a black hole is confined, to a flat-disk, a puffed disk, or a squirting jet. The GEMS project was cancelled in June 2012, projected to fail time and finance limits. The purpose of the GEMS mission continues to be relevant (as of 2019).

Space research on space stations

Soviet (later Russian) station Mir was the first long term inhabited station

Salyut 1

Salyut 1 was the first space station ever built. It was launched on April 19, 1971 by the Soviet Union. The first crew failed entry into the space station. The second crew was able to spend twenty-three days in the space station, but this achievement was quickly overshadowed since the crew died on reentry to Earth. Salyut 1 was intentionally deorbited six months into orbit since it prematurely ran out of fuel.[9]

Skylab

Skylab was the first American space station. It was 4 times larger than Salyut 1. Skylab was launched on May 14, 1973. It rotated through three crews of three during its operational time. Skylab's experiments confirmed coronal holes and were able to photograph eight solar flares.[10]

Mir

Soviet (later Russian) station Mir, from 1986 to 2001, was the first long term inhabited space station. Occupied in low Earth orbit for twelve and a half years, Mir served a permanent microgravity laboratory. Crews experimented with biology, human biology, physics, astronomy, meteorology and spacecraft systems. Goals included developing technologies for permanent occupation of space.

International Space Station

Main page: Astronomy:Scientific research on the International Space Station
The International Space Station of today is a modern research facility

The International Space Station received its first crew as part of STS-88, in December 1998, an internationally co-operative mission of almost 20 participants. The station has been continuously occupied for 23 years and 254 days, exceeding the previous record, almost ten years by Russian station Mir.[11] The ISS provides research in microgravity, and exposure to the local space environment. Crew members conduct tests relevant to biology, physics, astronomy, and others. Even studying the experience and health of the crew advances space research.

See also

Space view from Earth orbit


References

  1. A Brief History of High-Energy Astronomy: 1900-1958, NASA web page
  2. Willmore, Peter: COSPAR’s first 50 years, Public Lecture
  3. A Brief History of Space Exploration | The Aerospace Corporation. (n.d.). The Aerospace Corporation | Assuring Space Mission Success. Retrieved May 7, 2013
  4. COSPAR Scientific Structure, COSPAR web page
  5. Advances in Space Research, Elsevier web page
  6. UARS Science main page. (n.d.). UARS Science main page. Retrieved May 7
  7. ESA Science & Technology: Fact Sheet. (n.d.). ESA Science and Technology. Retrieved May 6, 2013
  8. GEMS
  9. Salyut 1 . (n.d.). Encyclopedia Astronautica. Retrieved May 7, 2013
  10. The SkyLab Project. (n.d.). Solar Physics Branch Home Page, Naval Research Laboratory. Retrieved May 7, 2013
  11. NASA - Facts and Figures. (n.d.). NASA - Home. Retrieved May 7, 2013

External links




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