Ultraviolet astronomy is the observation of
electromagnetic radiation
In physics, electromagnetic radiation (EMR) consists of waves of the electromagnetic (EM) field, which propagate through space and carry momentum and electromagnetic radiant energy. It includes radio waves, microwaves, infrared, (visible ...
at
ultraviolet
Ultraviolet (UV) is a form of electromagnetic radiation with wavelength from 10 nm (with a corresponding frequency around 30 PHz) to 400 nm (750 THz), shorter than that of visible light, but longer than X-rays. UV radiati ...
wavelengths between approximately 10 and 320
nanometre
330px, Different lengths as in respect to the Molecule">molecular scale.
The nanometre (international spelling as used by the International Bureau of Weights and Measures; SI symbol: nm) or nanometer ( American spelling) is a unit of length ...
s; shorter wavelengths—higher energy photons—are studied by
X-ray astronomy and
gamma-ray astronomy
Gamma-ray astronomy is the astronomical observation of gamma rays,Astronomical literature generally hyphenates "gamma-ray" when used as an adjective, but uses "gamma ray" without a hyphen for the noun. the most energetic form of electromagnet ...
.
Ultraviolet light is not visible to the
human eye. Most of the light at these wavelengths is absorbed by the Earth's atmosphere, so observations at these wavelengths must be performed from the upper atmosphere or from space.
Overview
Ultraviolet
line spectrum
The emission spectrum of a chemical element or chemical compound is the spectrum of frequencies of electromagnetic radiation emitted due to an electron making a transition from a high energy state to a lower energy state. The photon energy ...
measurements (
spectroscopy
Spectroscopy is the field of study that measures and interprets the electromagnetic spectra that result from the interaction between electromagnetic radiation and matter as a function of the wavelength or frequency of the radiation. Matter ...
) are used to discern the chemical composition, densities, and temperatures of the
interstellar medium
In astronomy, the interstellar medium is the matter and radiation that exist in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstella ...
, and the temperature and composition of hot young stars. UV observations can also provide essential information about the
evolution of galaxies
The study of galaxy formation and evolution is concerned with the processes that formed a heterogeneous universe from a homogeneous beginning, the formation of the first galaxies, the way galaxies change over time, and the processes that have gen ...
. They can be used to discern the presence of a hot
white dwarf
A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: its mass is comparable to the Sun's, while its volume is comparable to the Earth's. A white dwarf's faint luminosity comes ...
or
main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. These color-magnitude plots are known as Hertzsprung–Russell diagrams after their co-developers, Ejnar Her ...
companion in orbit around a cooler star.
[
The ultraviolet ]universe
The universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy. The Big Bang theory is the prevailing cosmological description of the development of the universe. A ...
looks quite different from the familiar star
A star is an astronomical object comprising a luminous spheroid of plasma held together by its gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night, but their immense distances from Earth make ...
s and galaxies
A galaxy is a system of stars, stellar remnants, interstellar gas, dust, dark matter, bound together by gravity. The word is derived from the Greek ' (), literally 'milky', a reference to the Milky Way galaxy that contains the Solar System. ...
seen in visible light
Light or visible light is electromagnetic radiation that can be perceived by the human eye. Visible light is usually defined as having wavelengths in the range of 400–700 nanometres (nm), corresponding to frequencies of 750–420 tera ...
.
Most stars are actually relatively cool objects emitting much of their electromagnetic radiation in the visible or near-infrared
Infrared (IR), sometimes called infrared light, is electromagnetic radiation (EMR) with wavelengths longer than those of visible light. It is therefore invisible to the human eye. IR is generally understood to encompass wavelengths from aroun ...
part of the spectrum. Ultraviolet radiation is the signature of hotter objects, typically in the early and late stages of their evolution
Evolution is change in the heritable characteristics of biological populations over successive generations. These characteristics are the expressions of genes, which are passed on from parent to offspring during reproduction. Variation ...
. In the Earth's sky seen in ultraviolet light, most stars would fade in prominence. Some very young massive stars and some very old stars and galaxies, growing hotter and producing higher-energy radiation near their birth or death, would be visible. Clouds of gas and dust would block the vision in many directions along the Milky Way
The Milky Way is the galaxy that includes our Solar System, with the name describing the galaxy's appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked ey ...
.
Space-based solar observatories such as SDO
A subdwarf O star (sdO) is a type of hot, but low-mass star. O-type subdwarfs are much dimmer than regular O-type main-sequence stars, but with a brightness about 10 to 100 times that of the Sun, and have a mass approximately half that of the Sun ...
and SOHO
Soho is an area of the City of Westminster, part of the West End of London. Originally a fashionable district for the aristocracy, it has been one of the main entertainment districts in the capital since the 19th century.
The area was develo ...
use ultraviolet telescopes (called AIA and EIT, respectively) to view activity on the Sun and its corona. Weather satellites such as the GOES-R series also carry telescopes
A telescope is a device used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. Originally meaning only an optical instrument using lenses, curved mirrors, or a combination of both to obser ...
for observing the Sun in ultraviolet.
The Hubble Space Telescope
The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most ver ...
and FUSE
Fuse or FUSE may refer to:
Devices
* Fuse (electrical), a device used in electrical systems to protect against excessive current
** Fuse (automotive), a class of fuses for vehicles
* Fuse (hydraulic), a device used in hydraulic systems to prote ...
have been the most recent major space telescope
A space telescope or space observatory is a telescope in outer space used to observe astronomical objects. Suggested by Lyman Spitzer in 1946, the first operational telescopes were the American Orbiting Astronomical Observatory, OAO-2 launch ...
s to view the near and far UV spectrum
A spectrum (plural ''spectra'' or ''spectrums'') is a condition that is not limited to a specific set of values but can vary, without gaps, across a continuum. The word was first used scientifically in optics to describe the rainbow of color ...
of the sky, though other UV instruments have flown on smaller observatories such as GALEX
Galaxy Evolution Explorer (GALEX or Explorer 83 or SMEX-7) was a NASA orbiting space telescope designed to observe the universe in ultraviolet wavelengths to measure the history of star formation in the universe. In addition to paving the ...
, as well as sounding rockets
A sounding rocket or rocketsonde, sometimes called a research rocket or a suborbital rocket, is an instrument-carrying rocket designed to take measurements and perform scientific experiments during its sub-orbital flight. The rockets are used to ...
and the Space Shuttle
The Space Shuttle is a retired, partially reusable low Earth orbital spacecraft system operated from 1981 to 2011 by the U.S. National Aeronautics and Space Administration (NASA) as part of the Space Shuttle program. Its official program na ...
.
Pioneers in ultraviolet astronomy include George Robert Carruthers
George Robert Carruthers (October 1, 1939 – December 26, 2020) was an African American inventor, physicist, engineer and space scientist. Carruthers perfected a compact and very powerful ultraviolet camera/spectrograph for NASA to use when ...
, Robert Wilson, and Charles Stuart Bowyer.
Ultraviolet space telescopes
* - Far Ultraviolet Camera/Spectrograph on Apollo 16 (April 1972)
* + ESRO
The European Space Research Organisation (ESRO) was an international organisation founded by 10 European nations with the intention of jointly pursuing scientific research in space. It was founded in 1964. As an organisation ESRO was based on a ...
- TD-1A (135-286 nm; 1972–1974)
* - Orbiting Astronomical Observatory (#2:1968-73. #3:1972-1981)
* - Orion 1 and Orion 2 Space Observatories
Orion () may refer to:
Common meanings
* Orion (constellation), named after the mythical hunter
* Orion (mythology), a hunter in Greek mythology
* Orion (spacecraft), NASA crew vehicle first launched in 2022
Arts and media
Fictional ent ...
(#1: 200-380 nm, 1971; #2: 200-300 nm, 1973)
* + - Astronomical Netherlands Satellite (150-330 nm, 1974–1976)
* + - International Ultraviolet Explorer (115-320 nm, 1978–1996)
* - Astron-1 (150-350 nm, 1983–1989)
* - Glazar 1 and 2 on Mir (in Kvant-1, 1987–2001)
* - EUVE (7-76 nm, 1992–2001)
* - FUSE
Fuse or FUSE may refer to:
Devices
* Fuse (electrical), a device used in electrical systems to protect against excessive current
** Fuse (automotive), a class of fuses for vehicles
* Fuse (hydraulic), a device used in hydraulic systems to prote ...
(90.5-119.5 nm, 1999–2007)
* + - Extreme ultraviolet Imaging Telescope (on SOHO
Soho is an area of the City of Westminster, part of the West End of London. Originally a fashionable district for the aristocracy, it has been one of the main entertainment districts in the capital since the 19th century.
The area was develo ...
imaging Sun at 17.1, 19.5, 28.4, and 30.4 nm)
* + - Hubble Space Telescope
The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most ver ...
(various 115-800 nm,1990-1997-) ( STIS 115–1030 nm, 1997–) ( WFC3 200-1700 nm, 2009–)
* - Swift Gamma-Ray Burst Mission (170–650 nm, 2004- )
* - Hopkins Ultraviolet Telescope (flew in 1990 and 1995)
* - ROSAT
ROSAT (short for Röntgensatellit; in German X-rays are called Röntgenstrahlen, in honour of Wilhelm Röntgen) was a German Aerospace Center-led satellite X-ray telescope, with instruments built by West Germany, the United Kingdom and the Uni ...
XUV (17-210eV) (30-6 nm, 1990–1999)
* - Far Ultraviolet Spectroscopic Explorer (90.5-119.5 nm, 1999–2007)
* - Galaxy Evolution Explorer (135–280 nm, 2003–2012)
* - Hisaki (130-530 nm, 2013 -)
* - Lunar-based ultraviolet telescope (LUT) (on Chang'e 3
Chang'e 3 (; ) is a robotic lunar exploration mission operated by the China National Space Administration (CNSA), incorporating a robotic lander and China's first lunar rover. It was launched in December 2013 as part of the second phase of ...
lunar lander, 245-340 nm, 2013 -)
* - Astrosat (130-530 nm, 2015 -)
* - Colorado Ultraviolet Transit Experiment
Colorado Ultraviolet Transit Experiment (CUTE) is a small UV space telescope to study selected exoplanets.
It was launched as a rideshare on the Atlas V that launched Landsat 9
Landsat 9 is an Earth observation satellite launched on 27 Sep ...
(CUTE) - (255-330 nm spectrograph, 2021- )
* - Public Telescope (PST) (100-180 nm, Proposed 2015, EU funded study )
* - Viewpoint-1 SpaceFab.US (200-950 nm, Launch planned 2022)
See also List of ultraviolet space telescopes
Ultraviolet instruments on planetary spacecraft
* - UVIS ('' Cassini'') - 1997 (at Saturn from 2004 to 2017)
* - MASCS (''MESSENGER
''MESSENGER'' was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. The name is a backronym for "Mercury Surface, Space Environment, Geoch ...
'') - 2004 (at Mercury from 2011 to 2015)
* - Alice (''New Horizons
''New Horizons'' is an interplanetary space probe that was launched as a part of NASA's New Frontiers program. Engineered by the Johns Hopkins University Applied Physics Laboratory (APL) and the Southwest Research Institute (SwRI), with a t ...
'') - 2006 (Pluto flyby in 2015)
* - UVS (''Juno'') - 2011 (at Jupiter since 2016)
* - IUVS (MAVEN
MAVEN is an American spacecraft orbiting Mars to study the loss of its atmospheric gases to space, providing insight into the history of
the planet's climate and water. The spacecraft name is an acronym for "Mars Atmosphere and Volatile Evolu ...
) - 2013 (at Mars since 2014)
See also
*
*
References
External links
*
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Astronomical imaging
Astronomical sub-disciplines
Astronomy
Astronomy () is a natural science that studies astronomical object, celestial objects and phenomena. It uses mathematics, physics, and chemistry in order to explain their origin and chronology of the Universe, evolution. Objects of interest ...