In astronomy, a green star is a white or blue star that appears green due to an optical illusion. There are no truly green stars, because the color of a star is more or less given by a black-body spectrum, which never looks green.[1] However, there are a few stars that appear green to some observers. This is usually because of the optical illusion that a red object can make nearby objects look greenish. There are some multiple star systems, such as Antares, with a bright red star where this illusion makes other stars in the system look green.
Why stars do not look green
The colors of black body radiation and most stars lie on the Planckian locus (the curved black line near the center of the diagram), with the corresponding temperature given in kelvins (in CIE 1931 x,y space). The spectral (rainbow) colors lie on the outer curved part of the diagram, with their wavelength given in nanometers.
Black body curves of Planck for various temperatures and comparison with classical theory of Rayleigh-Jeans.
A star is usually close to being a black body, give or take a few spectral lines, so its color is usually more or less the color of a black body. The color of a black body lies on the Planckian locus in the middle of the diagram shown here. As can be seen, this locus happens to pass through red, orange, yellow, white, and light blue areas, and one can indeed see many stars of these colors. On the other hand, it does not pass through green, indigo (dark blue) or violet areas, so stars that appear to have these colors are rare and depend on some additional optical effect.[2]
The (blackbody) colors of stars are sometimes confused with the colors of the spectrum. The spectral (rainbow) colors are those on the curved part of the boundary of the diagram on the right. As can be seen, the red, orange, yellow and blue rainbow colors happen to be much the same as blackbody colors. However, stars whose peak emission is green light also emit much red and blue light, and the human visual system happens to interpret this mixture of colors as whitish rather than green. So the fact that some spectral colors appear as star colors is more a quirk of human color vision than a property of stars: if one uses an instrument such as a spectroscope that is better at distinguishing wavelengths of light, then all spectral colors look completely different from star colors. All sufficiently hot stars look about the same shade of blue (and not violet as claimed in some popular accounts). The reason for this is that at sufficiently large temperatures (above about 20,000 K) all blackbody spectra look about the same in visible light, though they can differ a lot at shorter wavelengths. Although their maximum output at visible wavelengths is at violet, they put out enough light at other wavelengths to look light blue: the color at the end of the Planckian locus rather than the color at the end of the spectrum. Human color vision is in fact more complicated than suggested by the explanation above, and in particular the perceived color of an object depends not only on the light it emits, but also on the colors of nearby objects. For example, a blue object close to a red object may appear somewhat greenish; this effect accounts for many apparently green stars.
Objects that resemble green stars
Although there are no truly green stars, there are many astronomical objects that can sometimes appear to be green stars. This section lists some of them.
Multiple stars
Antares (red) and its companion star, Antares B
...there is no instance of an isolated deep blue or green star; these colors are apparently confined to the compound stars.
Elias Loomis, A Treatise on Astronomy, 1877, page 299
There a few stars in double or multiple star systems that appear greenish, even though they are really blue or white. This can happen if the star system contains a large red or orange star.[3] An optical illusion causes things close to the red star to appear slightly greenish.
The classical example is Antares B, the blue companion of the red supergiant Antares.[4]
Other examples include the star system Almach, and Sigma Cassiopeiae, a binary star 1500 light-years from Earth.
Sigma Cassiopeiae has a green-hued primary of magnitude 5.0 and a blue-hued secondary of magnitude 7.3.
Nebulae
The green planetary nebula NGC 6826
Some planetary nebulae glow green, especially if they contain oxygen. These nebulae, or the stars within them (usually Wolf-Rayet stars) may appear to be green stars. Some examples are the planetary nebulae NGC 6572, NGC 6826 and NGC 7009.
Beta Librae
Another mystery concerns the fact that this white star has so often been described as "greenish" or "pale emerald". Olcott refers to it as "the only naked-eye star that is green in color" while T.W.Webb refers to its "beautiful pale green hue". Star colors are strangely elusive, of course, and there are many such discrepancies in the guidebooks, but modern observers generally agree that the only stars which definitely appear green are the close companions to red stars such as Antares itself.
Burnham (1978, p.1105) discussing Zubeneschamali.
The star Beta Librae (Zubeneschamali) is usually reported to be white by modern observers.[5] However its color is controversial, and many earlier observers state that it is green.[6] There seems to be no consensus about what its color really is, and no generally accepted explanation for why some observers see it as green.[7]
Uranus
Uranus
The planet Uranus, occasionally mistaken for a star and once cataloged as one as 34 Tauri, can appear greenish as it has a lot of methane that absorbs red light.
The Sun
Green flash
The Sun can sometimes appear as a green spot for a second or two as it is rising or setting: this is known as green flash. Roughly speaking, the red light from the Sun is blocked by Earth, the blue light is scattered by the atmosphere, and the green light is refracted by the atmosphere to the observer.[8] A similar effect can occasionally be seen with other astronomical objects such as the moon and bright planets.
Furthermore, the Sun emits more green photons than any other color; i.e. it peaks in the green part of the visible spectrum.
False color images
The green blobs are false-color images of (non-green) stars.
Astronomical images are sometimes printed in false colors, which can make stars look green.
See also
Spectral classification
Sources
Burnham, Robert (1978). Burnham's celestial handbook: an observer's guide to the universe beyond the solar system. 2. New York: Dover. ISBN 9780486235684.
Feynman, Richard (1997). Surely you're joking, Mr. Feynman!. W. W. Norton & Company. ISBN 978-0-393-31604-9.
References
Fraser Cain (10 February 2009). "Are there Green Stars?". Universe Today – space and astronomy news. Retrieved 27 August 2017.
"Gröna stjärnor? Varför finns det inga gröna stjärnor?". Allt Om Vetenskap (in Swedish) (2). 9 October 2012. Archived from the original on 28 August 2017. Retrieved 27 August 2017.
Elias Loomis (1870). A Treatise on Astronomy. Harper and Brothers, New York.
Fred Schaaf (1983). Wonders of the Sky: Observing Rainbows, Comets, Eclipses, the Stars, and Other Phenomena. Courier Corporation. p. 213. ISBN 9780486244020. Retrieved 7 September 2017.
"Basic data: * bet Lib -- Variable star". Centre de Données astronomiques de Strasbourg. Retrieved 20 May 2015.
Robert Burnham (1978). Burnham's celestial handbook: an observer's guide to the universe beyond the solar system. 2. Dover, New York. p. 1105. ISBN 9780486235684. Retrieved 26 August 2017.
James B. Kaler (2006). "Zubeneschamali". Stars. University of Illinois. Archived from the original on 14 July 2006. Retrieved 26 August 2017.
Andrew T. Young. "Explaining Green Flashes". Retrieved 26 August 2017.
External links
Why are there no green stars? by Phil Plait
vte
Accretion Molecular cloud Bok globule Young stellar object
Protostar Pre-main-sequence Herbig Ae/Be T Tauri FU Orionis Herbig–Haro object Hayashi track Henyey track
Main sequence Red-giant branch Horizontal branch
Red clump Asymptotic giant branch
super-AGB Blue loop Protoplanetary nebula Planetary nebula PG1159 Dredge-up OH/IR Instability strip Luminous blue variable Blue straggler Stellar population Supernova Superluminous supernova / Hypernova
Early Late Main sequence
O B A F G K M Brown dwarf WR OB Subdwarf
O B Subgiant Giant
Blue Red Yellow Bright giant Supergiant
Blue Red Yellow Hypergiant
Yellow Carbon
S CN CH White dwarf Chemically peculiar
Am Ap/Bp HgMn Helium-weak Barium Extreme helium Lambda Boötis Lead Technetium Be
Shell B[e]
White dwarf
Helium planet Black dwarf Neutron
Radio-quiet Pulsar
Binary X-ray Magnetar Stellar black hole X-ray binary
Burster
Hypothetical
Blue dwarf Green Black dwarf Exotic
Boson Electroweak Strange Preon Planck Dark Dark-energy Quark Q Black Gravastar Frozen Quasi-star Thorne–Żytkow object Iron Blitzar
Deuterium burning Lithium burning Proton–proton chain CNO cycle Helium flash Triple-alpha process Alpha process Carbon burning Neon burning Oxygen burning Silicon burning S-process R-process Fusor Nova
Symbiotic Remnant Luminous red nova
Structure
Core Convection zone
Microturbulence Oscillations Radiation zone Atmosphere
Photosphere Starspot Chromosphere Stellar corona Stellar wind
Bubble Bipolar outflow Accretion disk Asteroseismology
Helioseismology Eddington luminosity Kelvin–Helmholtz mechanism
Properties
Designation Dynamics Effective temperature Luminosity Kinematics Magnetic field Absolute magnitude Mass Metallicity Rotation Starlight Variable Photometric system Color index Hertzsprung–Russell diagram Color–color diagram
Star systems
Binary
Contact Common envelope Eclipsing Symbiotic Multiple Cluster
Open Globular Super Planetary system
Earth-centric
observations
Sun
Solar System Sunlight Pole star Circumpolar Constellation Asterism Magnitude
Apparent Extinction Photographic Radial velocity Proper motion Parallax Photometric-standard
Lists
Proper names
Arabic Chinese Extremes Most massive Highest temperature Lowest temperature Largest volume Smallest volume Brightest
Historical Most luminous Nearest
Nearest bright With exoplanets Brown dwarfs White dwarfs Milky Way novae Supernovae
Candidates Remnants Planetary nebulae Timeline of stellar astronomy
Related articles
Substellar object
Brown dwarf Sub-brown dwarf Planet Galactic year Galaxy Guest Gravity Intergalactic Planet-hosting stars Tidal disruption event
Hellenica World - Scientific Library
Retrieved from "http://en.wikipedia.org/"
All text is available under the terms of the GNU Free Documentation License
