List of stars in Caelum
Encyclopedia
This is the list of notable star
s in the constellation
Caelum
, sorted by decreasing brightness.
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...
s in the constellation
Constellation
In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....
Caelum
Caelum
Caelum is a faint constellation in the southern sky, introduced in the 18th century by Nicolas Louis de Lacaille. Its name means "the chisel" in Latin, and it was formerly known as Cæla Sculptoris, "the sculptor's chisel"...
, sorted by decreasing brightness.
Name | B Bayer designation A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name... |
G. Gould designation Gould designations for stars are similar to Flamsteed designations in the way that they number stars within a constellation in increasing order of right ascension. Each star is assigned an integer , followed by " G. " , and then the Latin genitive of the constellation it lies in... |
HD Henry Draper Catalogue The Henry Draper Catalogue is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension , published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the... |
HIP | RA Right ascension Right ascension is the astronomical term for one of the two coordinates of a point on the celestial sphere when using the equatorial coordinate system. The other coordinate is the declination.-Explanation:... |
Dec Declination In astronomy, declination is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. Declination in astronomy is comparable to geographic latitude, but projected onto the celestial sphere. Declination is measured in degrees north and... |
vis. mag. Apparent magnitude The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere... |
abs. mag. Absolute magnitude Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth... |
Dist. (ly) | Sp. class Stellar classification In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure... |
Notes |
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α Cae Alpha Caeli Alpha Caeli is a double star system in the constellation Caelum.Alpha Caeli A is an F-type main sequence star with a stellar classification of F2V and an apparent magnitude of +4.44. It has 1.48 times the mass of the Sun and 1.3 times the solar radius. The projected rotational velocity at the... |
α | 9 | 29875 | 21770 | 4.44 | 2.92 | 66 | F2V | binary star Binary star A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary... |
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γ1 Cae | γ1 | 28 | 32831 | 23595 | 4.55 | 0.78 | 185 | K2III | binary star | ||
β Cae Beta Caeli Beta Caeli is a star in the constellation Caelum.β Caeli is a yellow-white F-type main sequence dwarf with an apparent magnitude of +5.04. It is approximately 90.2 light years from Earth and slightly over six times brighter than the Sun.... |
β | 10 | 29992 | 21861 | 5.04 | 2.83 | 90 | F3V | |||
δ Cae Delta Caeli Delta Caeli is a star in the constellation Caelum. It is a blue-white B-type subgiant with an apparent magnitude of +5.07. It is approximately 711 light years from Earth.-References:* *... |
δ | 7 | 28873 | 21060 | 5.07 | −1.62 | 710 | B2IV-V | |||
12 | 30080 | 21958 | 5.66 | −1.14 | 748 | K3III | |||||
19 | 31093 | 22573 | 5.82 | 1.10 | 286 | A2/A3V | binary star | ||||
26 | 32515 | 23446 | 5.92 | 0.90 | 329 | K2III | |||||
25 | 32453 | 23377 | 6.02 | 0.77 | 366 | G8III | |||||
15 | 30432 | 22144 | 6.04 | 1.12 | 315 | K1III | |||||
ν Cae Nu Caeli Nu Caeli is a star in the constellation Caelum.ν Caeli is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.06. It is approximately 171 light years from Earth.-References:* * *... |
ν | 18 | 30985 | 22488 | 6.06 | 2.47 | 171 | F1III-IV | double star Double star In observational astronomy, a double star is a pair of stars that appear close to each other in the sky as seen from Earth when viewed through an optical telescope. This can happen either because the pair forms a binary star, i.e... |
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3 | 28454 | 20781 | 6.10 | 3.54 | 106 | F8V | |||||
22 | 31529 | 22847 | 6.11 | −1.35 | 1012 | K3III | |||||
5 | 28700 | 20934 | 6.13 | 0.73 | 392 | K1III | |||||
λ Cae Lambda Caeli Lambda Caeli is a star in the constellation Caelum.λ Caeli is an orange K-type giant with an apparent magnitude of +6.24. It is approximately 652 light years from Earth.-References:* *... |
λ | 13 | 30202 | 21998 | 6.24 | −0.27 | 652 | K3/K4III | |||
27 | 32820 | 23555 | 6.30 | 3.82 | 102 | F8V | |||||
γ2 Cae | γ2 | 32846 | 23596 | 6.32 | 1.27 | 334 | F2IV/V | X Cae; δ Sct variable Delta Scuti variable A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the... , |
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ζ Cae Zeta Caeli Zeta Caeli is a star in the constellation Caelum.ζ Caeli is an orange K-type subgiant with an apparent magnitude of +6.35. It is approximately 514 light years from Earth.-References:* *... |
ζ | 16 | 30608 | 22280 | 6.35 | 0.36 | 513 | K0III | |||
1 | 28246 | 20630 | 6.38 | 3.54 | 121 | F6V | |||||
8 | 29559 | 21525 | 6.40 | 1.20 | 358 | A3Vs... | |||||
RV Cae RV Caeli RV Caeli is a variable star in the constellation Caelum.-References:* *... |
4 | 28552 | 20856 | 6.41 | −1.18 | 1072 | M1III | irregular variable Irregular variable An irregular variable is a type of variable star in which variations in brightness show no regular periodicity. There are two main sub-types of irregular variable: eruptive and pulsating.Eruptive irregular variables are divided into three categories:... , |