List of stars in Caelum
Encyclopedia
This is the list of notable star
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
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...

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...

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...

,
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:...

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