Giant and subgiant stars |
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Larger black and
white maps.
Often easier to see than even
the relatively "bright" AFGK
stars,
giant
stars located
within 100 light-years (ly)
-- 30.7 parsecs -- of Sol can
be prominent naked-eye
objects in Earth's night sky.
Summary
Within 100 light-years (or 30.7 parsecs) of Sol, there are around 34 confirmed giant stars and 213 possible subgiant stars (with another 24 or so possibly mis-classified dwarf stars). Subgiant stars are evolving off, or will "soon" leave, the "main sequence" because they are running out of hydrogen to sustain fusion at their cores. Most of these relatively bright but comparatively rare stars can be seen with the unaided Human eye in Earth's night sky.
Giant and Subgiant Stars within 100 Light-Years
Spectral Type | Giants | Probable Subgiants | |
O - Blue Stars | 0 | 0 | |
B - Blue-White Stars | 0 | 1 | |
A - Bluish White Stars | 5 | 17~ | |
F - Yellowish White Stars | 5 | 82~ | |
G - Yellow-Orange Stars | 5 | 77~ | |
K - Orange-Red Stars | 18 | 36~ | |
M - Red Stars | 1 | 0 | |
Total Giant and Subgiant Stars | 34 | 213~ |
Andrea
Dupree, Ronald Gilliland,
NASA and ESA
(Larger ultraviolet image --
more).
A highly evolved, orange-red giant star like
Arcturus
is still much smaller than the red supergiant
Betelgeuse,
at left. (See a Digitized Sky Survey
image of Arcturus from NASA's
NStars Database.)
While there are no giant stars located with 10 parsecs (or 33.3 light-years) of Sol, six stars -- Altair, Procyon A, Delta Pavonis, Beta Hydri, Mu Herculis Aa, and Rana -- appear to have already fused so much hydrogen and accumulated so much helium ash in their cores that they are beginning to swell and emit more yellow, orange, red, and infra-red light as subgiant stars -- shifting their spectral type towards the red end of the spectrum. As more massive stars exhaust their core hydrogen much faster, the largest O and B stars that may have once been born in the immediate 10-parsec, Solar neighborhood appear to have already moved off the main sequence and relatively brief, giant and supergiant stages to become white dwarfs and possibly as yet undetected neutron stars and black holes.
NASA
Observatorium
See a discussion of
the
"main
sequence"
as part of
stellar
evolution and death.
Arcturus is a nearby star located just outside the immediate 10-parsec Solar neighborhood (about 37 light-years away) that has already evolved out of the main sequence into giant status. Astronomers suspect that the star may have already shifted from the fusion of hydrogen to helium in its core, to the fusion of helium to carbon and oxygen, with trace activity of other nuclear processes, although Arcturus is somewhat brighter than expected for a stable helium-burning star (see Professor Jim Kaler's discussion). This helium-burning, orange-red giant stage is relatively brief, lasting tens to hundreds of million years (e.g., lasting around 700 million years for a star of one Solar mass like our Sun, Sol).
NASA
Observatorium
See a discussion of
"core
helium burning"
as part of
stellar
evolution and death.
Eventually, the star will lose much of its current mass, from an intensified stellar wind that eventually puffs out its outer gas envelopes of hydrogen and helium (and lesser amounts of higher elements such as carbon and oxygen) into interstellar space as a planetary nebula. The result will be a planet-sized, white dwarf core that gradually cools and fades in brightness from the shutdown of thermonuclear fusion. (Nearby white dwarfs include solitary Van Maanen's Star and the dim companions of Sirius, Procyon, and 40 (Omicron2) Eridani.)
H. Bond (STSci),
R. Ciardullo (PSU), WFPC2, HST, NASA
-- larger image
(White dwarfs are remnant stellar cores that have cast off their outer
gas
layers, like planetary nebula
NGC
2440.)
In March 2005, some astronomers announced that stars like Sol evolve through three stages that could foster life (see NASA news release with images). The first lasts for about 10 billion years, as the star burns hydrogen in its core during the main sequence. When the star exhausts its core hydrogen and begins to burn hydrogen in a shell around a growing helium core, it brightens and expands and becomes a "subgiant," during which its habitable zone moves outward with the increased heat radiated.
NASA
Larger image
As a Sol-type star
evolves beyond core
hydrogen fusion, it
brightens and expands
which moves its
habitable
zone
outwards
(more).
When our Sun, Sol, becomes a subgiant, its habitable zone may extending from two to nine AUs. Thus, the inner edge of this zone remains habitable for several billion years while the outer extreme, where Saturn currently orbits, is habitable for a few hundred million years. The star then fluctuates in brightness for about 20 million years as it switches to core helium burning almost exclusively, before becoming a red giant and swelling to around 10 times the diameter of the Sun.
NASA
Larger image
When Sol becomes
a giant star, its
habitable zone
will extend from
7 to 22 AUs -- an
outer edge beyond
the orbit of Uranus.
For about a billion years afterwards, the habitable zone around the red giant extends from 7 to 22 AU, the outer edge of which lies beyond the orbit of Uranus. Hence, planets that are currently very cold and icy can warm up and become potentially habitable. The time period over which these conditions change may be long enough for life to develop. Moreover, bacteria could be transported by meteorites from an inner planet where life is ending to an outer planet where conditions are warming up.
Nearby Giant Stars by Brightness, Spectra, and Distance
The following giant stars are located within 100 light-years (ly), 30.7 parsecs, of Sol.
Nearby Subgiant Stars by Brightness, Spectra, and Distance
The following suspected subgiant stars are located within 100 light-years (ly), 30.7 parsecs, of Sol.
Other Information
Summary information on main sequence, blue-white B, bluish white A, yellowish F, yellow-orange G, orange-red K , and many red M stars within 100 light-years are also available.
Try Professor James Kaler's Stars for more information on giant, supergiant, and prominent subgiant stars. See also a paper on the use of subgiant stars to date the oldest stars of Milky Way disk from Sandage et al, 2003.
Up-to-date technical summaries on some stars can be found at: NASA Star and Exoplanet Database, the Astronomiches Rechen-Institut at Heidelberg's ARCNS, Centre de Données astronomiques de Strasbourg's SIMBAD, and www.alcyone.de's bright star catalogue search. Additional information may be available at Roger Wilcox's Internet Stellar Database.
For more information about stars including spectral and luminosity class codes, go to ChView's webpage on The Stars of the Milky Way.
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