Astronomy:Green star

From HandWiki

In astronomy, a green star is a white or blueish star that appears greenish in some viewing conditions (see 'Psychology' below). Under typical viewing conditions, there are no greenish stars, because the color of a star is more or less given by a black-body spectrum.[1] However, there are a few stars that appear greenish to some observers, due to the viewing conditions, for example the optical 'illusion' that a red object can make nearby objects look greenish (and vice versa). Some multiple star systems, such as Antares, have a bright reddish star where this contrast makes other stars in the system look more green.

Psychology of color perception

All color vision is created by the brain of the observer. As such, no star really has any colour at all. Therefore color is not a fundamental property, it is in the brain of the observer. Stars emit energy at many different wavelengths, and humans may perceive color in stars. Instead of talking about the 'true' color of stars, we must talk about how a particular object appears to a particular observer, in a particular context. This is not mere semantics: green can be perceived when there is no 'green' light at all - for example due to the simultaneous colour contrast[2][3] alluded to above, in that a star can look greenish when it is next to a reddish star (likewise, the reddish star will appear more red when next to a non-reddish star). Green percepts can also be created by blocking red light, and by adapting the 'red' photoreceptors (see complementary colors). This is not an 'illusion', this is simply how humans perceive colour. The perception of colour in stars is complicated by the fact that the cone photoreceptors, from which colour percepts are typically generated, are not active during the dim lighting conditions required to see most stars without magnification - that is, in scotopic vision. Further, stars are effectively single points of light at vast distances from the observer's eye; this light is filtered through the atmosphere, through pollution, through the eye and the brain. It is only because starlight is split, scattered, and/or because the observer's eye is always moving, that the light from a star can stimulate multiple photoreceptors in the retina, and therefore generate percepts of colour, relative to the background illumination.

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.[4]

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.

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 are a few stars in double or multiple star systems that appear greenish, even though they are blue or white under typical viewing conditions. This can happen if the star system contains a large red or orange star.[5] Colour contrast effects result in objects close to the reddish star appear slightly greenish (and vice versa: complementary colors).

The classical example is Antares B, the blue companion of the red supergiant Antares.[6]

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.


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) discussing Zubeneschamali.

The star Beta Librae (Zubeneschamali) is usually reported to be white by modern observers.[7] However its color is controversial, and many earlier observers state that it is green.[8] 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.[9]



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.[10] 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



  1. Fraser Cain (10 February 2009). "Are there Green Stars?". Universe Today – space and astronomy news. 
  2. Daw, Nigel W. (17 November 1967). "Goldfish Retina: Organization for Simultaneous Colour Contrast". Science 158 (3803): 942–4. doi:10.1126/science.158.3803.942. PMID 6054169. Bibcode1967Sci...158..942D. 
  3. Bevil R. Conway (2002). Neural Mechanisms of Color Vision: Double-Opponent Cells in the Visual Cortex. Springer. ISBN 978-1-4020-7092-1. 
  4. "Gröna stjärnor? Varför finns det inga gröna stjärnor?" (in sv). Allt Om Vetenskap (2). 9 October 2012. Retrieved 27 August 2017. 
  5. Elias Loomis (1870). A Treatise on Astronomy. Harper and Brothers, New York. 
  6. 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. 
  7. "Basic data: * bet Lib -- Variable star". Centre de Données astronomiques de Strasbourg. 
  8. 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. 
  9. James B. Kaler (2006). "Zubeneschamali". Stars. University of Illinois. 
  10. Andrew T. Young. "Explaining Green Flashes". 

External links