List of stars in Camelopardalis
Encyclopedia
This is the list of notable star
s in the constellation
Camelopardalis
, 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....
Camelopardalis
Camelopardalis
Camelopardalis is a large but faint constellation in the northern sky. The constellation was introduced in 1612 by Petrus Plancius. Some older astronomy books give an alternative spelling of the name, Camelopardus.-Etymology:...
, 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... |
F Flamsteed designation Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and 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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β Cam Beta Camelopardalis Beta Camelopardalis is a star in the constellation Camelopardalis.β Camelopardalis is a yellow G-type supergiant with an apparent magnitude of +4.03. This is a double star, with components of magnitudes 4.0 and 7.4. It is approximately 1000 light years from Earth.-References:* * *... |
β | 10 | 31910 | 23522 | 4.03 | −3.40 | 997 | G0Ib | |||
CS Cam CS Camelopardalis CS Camelopardalis is a binary star in reflection nebulae vdB 14, in the constellation Camelopardalis. It was designated B Cam or 2H.Cam.... |
B | 21291 | 16228 | 4.21 | −6.39 | 4289 | B9Ia | α Cyg variable Alpha Cygni variable Alpha Cygni variables are variable stars which exhibit non-radial pulsations, meaning that some portions of the stellar surface are contracting at the same time others parts expand. They are supergiant stars of spectral types B or A... |
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α Cam Alpha Camelopardalis Alpha Camelopardalis is an O-type supergiant star, with an apparent visual magnitude of approximately 4.301. It is the third brightest star in the constellation of Camelopardalis, the first and second brightest being β Camelopardalis and CS Camelopardalis, respectively... |
α | 9 | 30614 | 22783 | 4.26 | −7.38 | 6936 | O9.5Ia SB: | Shǎowèi (少衛) | ||
BE Cam BE Camelopardalis BE Camelopardalis is a star in the constellation Camelopardalis.BE Camelopardalis is a red M-type bright giant with a mean apparent magnitude of +4.39. It is approximately 965 light years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +4.35 to... |
23475 | 17884 | 4.39 | −2.97 | 964 | 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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7 Cam 7 Camelopardalis 7 Camelopardalis is a triple star system in the constellation Camelopardalis. It is approximately 376 light years from Earth.The primary component, 7 Camelopardalis A, is a white A-type main sequence dwarf with an apparent magnitude of +4.43... |
7 | 31278 | 23040 | 4.43 | −0.88 | 376 | A1V | ||||
CE Cam CE Camelopardalis CE Camelopardalis is a variable star in reflection nebula VDB 15, in the constellation Camelopardalis.-References:* *... |
C | 21389 | 16281 | 4.55 | −4.85 | 2470 | A0Ia SB: | ||||
M Cam M Camelopardalis M Camelopardalis is a star in the constellation Camelopardalis.M Camelopardalis is an orange K-type giant with an apparent magnitude of +4.55. It is approximately 187 light years from Earth.-References:* *... |
M | 49878 | 33694 | 4.55 | 0.76 | 187 | K4III | ||||
γ Cam Gamma Camelopardalis Gamma Camelopardalis is a star in the constellation Camelopardalis.γ Camelopardalis is a white A-type subgiant with an apparent magnitude of +4.59. It is approximately 335 light years from Earth.-References:* *... |
γ | 23401 | 17959 | 4.59 | −0.47 | 335 | A2IVn | ||||
BK Cam BK Camelopardalis BK Camelopardalis is a variable star in the Camelopardalis.-Chinese name:In Chinese, , meaning Right Wall of Purple Forbidden Enclosure, refers to an asterism consisting of BK Camelopardalis, α Draconis, κ Draconis, λ Draconis, 24 Ursae Majoris, 43 Camelopardalis and α Camelopardalis... |
A | 20336 | 15520 | 4.74 | −2.21 | 801 | B2.5Vne | ||||
L Cam HD 42818 HD 42818 is a star in the constellation Camelopardalis.HD 42818 is a white A-type main sequence dwarf with an apparent magnitude of +4.76. It is approximately 176 light years from Earth.... |
L | 42818 | 29997 | 4.76 | 1.10 | 176 | A0Vn | ||||
PLX 772 | 23089 | 17587 | 4.78 | −2.17 | 799 | A3V... | |||||
VZ Cam VZ Camelopardalis VZ Camelopardalis is a Semiregular variable star in the constellation Camelopardalis.VZ Camelopardalis is a M-type red giant with a mean apparent magnitude of +4.92. It is approximately 473 light years from Earth... |
55966 | 36547 | 4.92 | −0.89 | 473 | M4IIIa | semiregular variable | ||||
H Cam | H | 24479 | 18505 | 4.95 | −0.13 | 338 | B9.5V | ||||
24480 | 18488 | 4.99 | −3.78 | 1852 | K3I-II | ||||||
25291 | 19018 | 5.00 | −3.63 | 1734 | F0II | ||||||
BD Cam BD Camelopardalis BD Camelopardalis is an S star and symbiotic star in the constellation Camelopardalis. It was recognized as a spectroscopic binary star in 1922, and its orbital solution published in 1984; it has a 596-day orbital period... |
22649 | 17296 | 5.06 | −0.95 | 520 | S5.3 SB: | a symbiotic star | ||||
3 Cam | 3 | 29317 | 21727 | 5.07 | −0.84 | 495 | K0III SB | Cepheid variable Cepheid variable A Cepheid is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period, secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.Cepheid... |
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K Cam HD 33564 HD 33564 is a 5th magnitude star located approximately 48 light-years away in the constellation of Camelopardalis. It is an F-type main sequence, indicating that the star is hotter and more massive than our Sun. The age of the star is only 3 Ga; despite of this, the star is only 76% the solar... |
K | 33564 | 25110 | 5.08 | 3.47 | 68 | F6V | has a planet Extrasolar planet An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars... (b HD 33564 b HD 33564 b is an extrasolar planet located approximately 68 light-years away in the constellation of Camelopardalis. This planet orbits around F6V star HD 33564. The planet has an eccentric eccentric orbit, ranging in distance from 0.737 AU at periastron to 1.497 AU at apastron.... ) |
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SV ZI 191 | D | 21447 | 16292 | 5.09 | 1.25 | 191 | A1V | ||||
43 Cam 43 Camelopardalis 43 Camelopardalis is a star in the constellation Camelopardalis.43 Camelopardalis is a blue-white B-type giant with an apparent magnitude of +5.11... |
43 | 49340 | 33104 | 5.11 | −2.32 | 1000 | B7III | ||||
CQ Cam CQ Camelopardalis CQ Camelopardalis is a variable star in the constellation Camelopardalis.-References:* *... |
20797 | 15890 | 5.13 | −2.79 | 1249 | M0II | variable star Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth... |
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42 Cam 42 Camelopardalis 42 Camelopardalis is a star in the constellation Camelopardalis.42 Camelopardalis is a blue-white variable B-type subgiant with an apparent magnitude of +5.14... |
42 | 48879 | 32864 | 5.14 | −1.98 | 867 | B4IV | ||||
CO Cam | N | 106112 | 59504 | 5.14 | 2.50 | 110 | A5m | ||||
26764 | 19949 | 5.20 | 0.03 | 353 | A2Vn | ||||||
31 Cam 31 Camelopardalis 31 Camelopardalis is an eclipsing spectroscopic binary in the constellation Camelopardalis. It is approximately 405 light years from Earth.... |
31 | 39220 | 27971 | 5.20 | −0.27 | 405 | A2V | TU Cam; eclipsing spectroscopic binary | |||
11 Cam 11 Camelopardalis 11 Camelopardalis or BV Camelopardalis is a star system in the constellation Camelopardalis. It forms a double star with 12 Camelopardalis, which is only 3 arcminutes away.... |
11 | 32343 | 23734 | 5.22 | −1.35 | 671 | B2.5Ve | BV Cam; γ Cas variable; 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... with 12 Cam |
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16 Cam 16 Camelopardalis 16 Camelopardalis is a star in double system in the constellation Camelopardalis.-References:* * * -Components:... |
16 | 34787 | 25197 | 5.24 | 0.15 | 340 | A0Vn | ||||
NSV 4864 | 90089 | 51502 | 5.25 | 3.59 | 70 | F2V | |||||
27022 | 20266 | 5.26 | 0.22 | 333 | G5III | ||||||
4 Cam 4 Camelopardalis 4 Camelopardalis is a star in double system in the constellation Camelopardalis.-References:* * *... |
4 | 30121 | 22287 | 5.29 | 1.81 | 162 | A3m | ||||
37 Cam | 37 | 41597 | 29246 | 5.35 | 0.20 | 349 | G8III | ||||
2 Cam 2 Camelopardalis 2 Camelopardalis is a double or multiple star in the constellation Camelopardalis.- References :* * * - Components :... |
2 | 29316 | 21730 | 5.36 | 0.71 | 277 | A8V | multiple star Multiple star A multiple star consists of three or more stars which appear from the Earth to be close to one another in the sky. This may result from the stars being physically close and gravitationally bound to each other, in which case it is physical, or this closeness may be merely apparent, in which case... |
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36 Cam | 36 | 41927 | 29490 | 5.36 | −1.11 | 642 | K2II-III | ||||
40 Cam 40 Camelopardalis 40 Camelopardalis is a star in double system in the constellation Camelopardalis.-References:* * *... |
40 | 42633 | 29730 | 5.37 | −0.55 | 498 | K3III | ||||
64307 | 39117 | 5.37 | −1.29 | 700 | K3III | ||||||
Σ 1694 | 112028 | 62572 | 5.38 | 0.54 | 303 | A1IIIsh | |||||
64486 | 39538 | 5.39 | 0.36 | 330 | A0p... | ||||||
23277 | 17854 | 5.40 | 0.40 | 325 | A2m | ||||||
NSV 1558 | 27245 | 20376 | 5.40 | −0.18 | 427 | M0III | |||||
17 Cam 17 Camelopardalis 17 Camelopardalis is variable star in the constellation Camelopardalis.-References:* *... |
17 | 35583 | 25769 | 5.43 | −1.85 | 931 | M1III | ||||
BN Cam BN Camelopardalis BN Camelopardalis is a Alpha² Canum Venaticorum variable star in the constellation Camelopardalis.-References:* *... |
32650 | 24254 | 5.44 | 0.14 | 374 | B9p Si | α2 CVn variable | ||||
46588 | 32439 | 5.44 | 4.18 | 58 | F8V | ||||||
30442 | 22626 | 5.47 | −0.46 | 499 | M2III | ||||||
5 Cam 5 Camelopardalis 5 Camelopardalis is a star in double system in the constellation Camelopardalis.-References:* * *... |
5 | 30958 | 22854 | 5.52 | −1.02 | 661 | B9.5V | ||||
89571 | 51384 | 5.52 | 2.47 | 133 | F0IV | ||||||
68375 | 40793 | 5.55 | 0.79 | 292 | G8III | ||||||
37289 | 26882 | 5.62 | 0.96 | 279 | K5III | ||||||
58425 | 36528 | 5.63 | −0.08 | 453 | K2III | ||||||
34255 | 24914 | 5.64 | −3.27 | 1976 | K4Iab: | ||||||
26670 | 19968 | 5.69 | 0.20 | 409 | B5Vn | ||||||
50885 | 33827 | 5.69 | −0.04 | 457 | K4III | ||||||
26755 | 19983 | 5.72 | 1.18 | 263 | K1III | ||||||
22764 | 17342 | 5.74 | −3.41 | 2203 | K4Ib | ||||||
117566 | 65595 | 5.74 | 0.98 | 292 | G2.5IIIb | ||||||
31134 | 22936 | 5.75 | −0.08 | 478 | A2Vs | ||||||
45866 | 31940 | 5.75 | −0.50 | 579 | K5III | ||||||
DL Cam DL Camelopardalis DL Camelopardalis is a variable star in the constellation Camelopardalis.... |
1 | 28446 | 21148 | 5.78 | B0III SB | variable star Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth... |
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HD 104985 HD 104985 |- bgcolor="#FFFAFA"HD 104985 is a helium-fusing yellow giant star in the constellation of Camelopardalis. It is located 333 ly or 102 parsecs away from Earth. In 2003, an extrasolar planet was discovered in orbit around the star.... |
104985 | 58952 | 5.78 | 0.74 | 333 | G9III | has a planet (b HD 104985 b HD 104985 b is an extrasolar planet that takes 198 days to orbit at the distance of 0.78 AU. It is definitely a gas giant since it has mass 61/3 times Jupiter.- External links :*... ) |
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23005 | 17585 | 5.79 | 2.07 | 181 | F0IV | ||||||
24141 | 18217 | 5.80 | 2.21 | 170 | A5m | ||||||
33541 | 24732 | 5.81 | 0.60 | 359 | A0V | ||||||
23523 | 17891 | 5.82 | 1.57 | 231 | A5Vn | ||||||
25274 | 19129 | 5.88 | −0.53 | 623 | K2III | ||||||
46509 | 31946 | 5.88 | −0.66 | 663 | K0III | ||||||
27322 | 20380 | 5.91 | 1.02 | 310 | A3V | ||||||
28780 | 21452 | 5.91 | 0.24 | 443 | A1V | ||||||
112014 | 62561 | 5.92 | 1.75 | 222 | A0V | ||||||
120565 | 66878 | 5.92 | 0.68 | 364 | G9III | ||||||
26 Cam 26 Camelopardalis 26 Camelopardalis is a star in the constellation Camelopardalis.26 Camelopardalis is a white A-type main sequence dwarf with an apparent magnitude of +5.93. It is approximately 193 light years from Earth.... |
26 | 38091 | 27249 | 5.93 | 2.07 | 193 | A4Vn | ||||
51 Cam | 51 | 62066 | 37949 | 5.93 | 0.89 | 332 | K2III: | ||||
28204 | 21247 | 5.94 | 0.65 | 373 | A8m | ||||||
29678 | 22361 | 5.96 | 2.66 | 149 | A9IV | ||||||
21819 | 16599 | 5.98 | 1.82 | 222 | A3V | ||||||
32356 | 23766 | 6.00 | −0.19 | 563 | K5II | ||||||
105943 | 59384 | 6.00 | −1.64 | 1101 | K5III: | ||||||
53 Cam 53 Camelopardalis 53 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 321 light years from Earth. The binary has an orbital period of 6.52 years.... |
53 | 65339 | 39261 | 6.02 | 1.05 | 321 | A2p... | AX Cam; α2 CVn variable Alpha2 Canum Venaticorum variable An Alpha2 Canum Venaticorum variable is a type of variable star. These stars are chemically peculiar main sequence stars of spectral class B8p to A7p. They have strong magnetic fields and strong silicon, strontium, or chromium spectral lines... ; spectroscopic binary |
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31662 | 23380 | 6.03 | 3.19 | 120 | F4V | ||||||
44472 | 30794 | 6.03 | −0.12 | 553 | A4V | ||||||
26076 | 19730 | 6.05 | 0.80 | 365 | K1III | ||||||
31312 | 23442 | 6.05 | −0.37 | 628 | K5III | ||||||
24 Cam | 24 | 37601 | 26942 | 6.05 | 2.11 | 200 | K0III | ||||
26553 | 19823 | 6.06 | −1.96 | 1309 | A4III | ||||||
12 Cam 12 Camelopardalis 12 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It also forms a double star with 11 Camelopardalis, which is only 3 arcminutes away.... |
12 | 32357 | 23743 | 6.08 | −0.33 | 625 | K0III | BM Cam; RS CVn variable RS Canum Venaticorum variable RS Canum Venaticorum variables are a type of variable star. They are close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity... ; double star with 11 Cam |
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23383 | 17707 | 6.09 | 0.48 | 431 | B9Vnn | ||||||
8 Cam | 8 | 31579 | 23216 | 6.09 | −0.77 | 767 | K4III | ||||
65448 | 39340 | 6.09 | 0.07 | 522 | G1III | ||||||
31590 | 23617 | 6.10 | 0.02 | 537 | A1V | ||||||
99945 | 56253 | 6.12 | 2.24 | 195 | A2m | ||||||
15 Cam | 15 | 34233 | 24836 | 6.13 | −1.02 | 879 | B5V | DV Cam; Algol variable Algol variable Algol variables or Algol-type binaries are a class of eclipsing binary stars where the orbital plane of the stars are coincident with the line of sight from Earth. When the cooler component passes in front of the hotter one, part of the latter's light is blocked, and the total brightness of the... |
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21427 | 16303 | 6.14 | 1.07 | 337 | A2V | ||||||
25425 | 19177 | 6.14 | 0.41 | 457 | A3m | ||||||
30 Cam | 30 | 38831 | 27731 | 6.14 | 0.02 | 545 | A0Vs | ||||
33618 | 24479 | 6.15 | 1.28 | 307 | K2III-IV | ||||||
19 Cam | 19 | 36570 | 26408 | 6.15 | 0.86 | 372 | A0V | ||||
72582 | 42484 | 6.16 | 0.97 | 355 | G7III | ||||||
33266 | 24313 | 6.17 | 0.34 | 477 | A2III | ||||||
23 Cam | 23 | 37638 | 27046 | 6.17 | 1.23 | 318 | G5III: | ||||
27402 | 20456 | 6.18 | 0.86 | 378 | A4V | ||||||
38284 | 27472 | 6.18 | 0.67 | 412 | A4V | ||||||
36384 | 26638 | 6.19 | −0.06 | 579 | M0III | ||||||
31675 | 23484 | 6.20 | 3.97 | 91 | F6V: | ||||||
31563 | 23582 | 6.21 | −1.84 | 1331 | K0 | ||||||
FR Cam | 104216 | 58545 | 6.21 | −0.79 | 819 | M2III | |||||
38645 | 27795 | 6.22 | 0.70 | 415 | G9III | ||||||
39429 | 28205 | 6.24 | 0.66 | 427 | K0 | ||||||
25948 | 19400 | 6.25 | 2.87 | 155 | F5V | ||||||
115337 | 64437 | 6.25 | −0.37 | 686 | K0Ib | ||||||
36496 | 26410 | 6.26 | 1.76 | 259 | A8Vn | ||||||
45947 | 31703 | 6.26 | 3.51 | 116 | F2 | ||||||
104904 | 58874 | 6.27 | 1.86 | 249 | F6V | ||||||
27855 | 20772 | 6.28 | −0.54 | 755 | A0III | ||||||
40055 | 28831 | 6.28 | −0.44 | 720 | K5 | ||||||
67934 | 41208 | 6.28 | −0.31 | 679 | A2Vn | ||||||
KZ Cam | 22316 | 16974 | 6.29 | 0.13 | 557 | B9p | HR 1094; α² CVn variable | ||||
25877 | 19412 | 6.29 | −1.30 | 1072 | G8II | ||||||
55075 | 36019 | 6.30 | −0.73 | 832 | A0III | ||||||
76990 | 45421 | 6.30 | 1.53 | 294 | F2III | ||||||
23662 | 18067 | 6.31 | −0.70 | 821 | B9IVp | ||||||
24164 | 18438 | 6.31 | 2.42 | 196 | A5m | ||||||
25602 | 19172 | 6.31 | 1.36 | 319 | K0III-IV | ||||||
71973 | 42249 | 6.31 | 1.69 | 273 | A2m | ||||||
86321 | 49688 | 6.31 | −0.85 | 883 | K0 | ||||||
30144 | 22300 | 6.32 | 2.78 | 166 | F0 | ||||||
40827 | 28829 | 6.32 | 0.52 | 471 | K1III-IV | ||||||
26101 | 19673 | 6.33 | 0.96 | 387 | K0 | ||||||
111112 | 62170 | 6.33 | 0.57 | 462 | A5m | ||||||
30085 | 22508 | 6.36 | −0.13 | 647 | A0IV | ||||||
32781 | 24440 | 6.36 | 0.81 | 421 | A0V | ||||||
54070 | 34956 | 6.36 | 0.94 | 396 | K0 | ||||||
47 Cam | 47 | 56820 | 35735 | 6.36 | 2.13 | 229 | A8m | ||||
21794 | 16602 | 6.37 | 2.09 | 234 | F7V | ||||||
32715 | 24017 | 6.37 | 3.38 | 129 | F3V: | ||||||
77246 | 45097 | 6.37 | 1.93 | 252 | F2 | ||||||
34200 | 24955 | 6.39 | 1.04 | 384 | G5 | ||||||
30752 | 22720 | 6.40 | 0.37 | 523 | A2V | ||||||
69054 | 41011 | 6.40 | 0.63 | 466 | K0III... | ||||||
20104 | 15309 | 6.41 | 0.10 | 596 | A3V | ||||||
40956 | 28951 | 6.42 | 0.90 | 414 | K0 | ||||||
79517 | 45764 | 6.42 | 1.14 | 370 | G8III | ||||||
21903 | 16712 | 6.43 | 2.69 | 183 | F5V | ||||||
HD 32518 HD 32518 HD 32518 is a 6th magnitude K-type giant star located approximately 390 light years away in the constellation of Camelopardalis. It is 1.13 times more massive, 10.22 times larger, and 41.2 times more luminous than the Sun. However, it has a lower amount of metals than our Sun and the age is older.... |
32518 | 24003 | 6.44 | 1.09 | 383 | K1III | has a planet (b HD 32518 b HD 32518 b is an extrasolar planet which orbits the K-type giant star HD 32518, located approximately 383 light years away in the constellation Camelopardalis. It has a minimum mass three times greater than Jupiter and orbits the intermediate-mass giant star at a distance of only 0.59 AU in a very... ) |
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18 Cam | 18 | 36066 | 25973 | 6.44 | 3.23 | 143 | F8V | ||||
21769 | 16587 | 6.45 | −0.40 | 763 | A4III | ||||||
65299 | 40559 | 6.45 | 0.24 | 568 | A3IV | ||||||
23594 | 17858 | 6.46 | 0.40 | 531 | A0Vn | ||||||
29329 | 22152 | 6.46 | 3.92 | 105 | F7V | ||||||
118686 | 66251 | 6.46 | −1.03 | 1025 | K5III: | ||||||
57742 | 36211 | 6.47 | −0.72 | 893 | B9III | ||||||
34450 | 25322 | 6.48 | −1.45 | 1254 | M0 | ||||||
41782 | 29348 | 6.48 | −1.47 | 1268 | M0 | ||||||
21203 | 16177 | 6.49 | −0.61 | 858 | B9V | ||||||
25225 | 19222 | 6.49 | 1.00 | 409 | K0 | ||||||
14 Cam | 14 | 33296 | 24348 | 6.49 | 1.91 | 268 | A7Vn | ||||
38058 | 27346 | 6.49 | 0.64 | 482 | G5 | ||||||
52030 | 34238 | 6.49 | −0.58 | 847 | K0III | ||||||
40568 | 28656 | 6.50 | 0.31 | 565 | G5 | ||||||
49 Cam 49 Camelopardalis 49 Camelopardalis is a star in the constellation Camelopardalis.49 Camelopardalis is a yellow-white F-type main sequence dwarf with a mean apparent magnitude of +6.50. It is approximately 265 light years from Earth. It is classified as an Alpha2 Canum Venaticorum type variable star and its... |
49 | 62140 | 37934 | 6.50 | 1.95 | 265 | F0p SrEu | BC Cam; α2 CVn variable | |||
29 Cam | 29 | 38618 | 27592 | 6.53 | 0.88 | 441 | A4IV-V | ||||
28 Cam 28 Camelopardalis 28 Camelopardalis is a star in the constellation Camelopardalis.28 Camelopardalis is a white A-type main sequence dwarf with an apparent magnitude of +6.79. It is approximately 622 light years from Earth.... |
28 | 38129 | 27283 | 6.79 | 0.39 | 622 | A7V | ||||
22 Cam 22 Camelopardalis 22 Camelopardalis is a star in the constellation Camelopardalis.22 Camelopardalis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +7.03. It is approximately 196 light years from Earth.... |
22 | 37070 | 26587 | 7.03 | 3.14 | 196 | F5 |