Upsilon Carinae

Not to be confused with Y Carinae.
υ Carinae
Location of υ Carinae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 09h 47m 06.12170s[1]
Declination –65° 04′ 19.2267″[1]
Apparent magnitude (V) 2.97[2] (+3.08/+6.25[3])
Characteristics
Spectral type A8 Ib + B7 III[4]
U−B color index +0.13[2]
B−V color index +0.27[2]
Astrometry
Radial velocity (Rv)+14[4] km/s
Proper motion (μ) RA: –11.51[1] mas/yr
Dec.: +4.71[1] mas/yr
Parallax (π)2.27 ± 0.28 mas[1]
Distanceapprox. 1,400 ly
(approx. 440 pc)
Absolute magnitude (MV)−5.26[5]
Details
υ Car A
Mass13[4] M☉
Surface gravity (log g)1.1 ± 0.3[4] cgs
Temperature7,600 ± 350[4] K
Age12[6] Myr
υ Car B
Mass8[4] M☉
Surface gravity (log g)3.3 ± 0.1[4] cgs
Temperature23,000 ± 1600[4] K
Other designations
υ Car, CP−64°1084, HIP 48002[7]
A: HD 85124, HR 3891, SAO 250696
B: HD 85123, HR 3890, SAO 250695
Database references
SIMBADsystem
A
B

Upsilon Carinae, Latinized from υ Carinae, is a double star in the southern constellation of Carina. It is part of the Diamond Cross asterism in southern Carina. The Upsilon Carinae system has a combined apparent magnitude of +2.97[2] and is approximately 1,400 light years (440 parsecs) from Earth.[1]

In Chinese, 海石 (Hǎi Dàn), meaning Sea Rock, refers to an asterism consisting of υ Carinae, ε Carinae, ι Carinae, HD 83183 and HD 84810.[8] Consequently, υ Carinae itself is known as 海石五 (Hǎi Dàn wǔ, English: the Fifth Star of Sea Rock.)[9]

The primary component, υ Carinae A, has a stellar classification of A8 Ib, making it a supergiant star that has exhausted the hydrogen at its core and evolved away from its brief main sequence lifetime as an O9 V star.[4] With an apparent magnitude of +3.08,[3] it has an effective temperature of about 7,600 K,[4] giving it a white hue. The companion, υ Carinae B, is a giant star with a classification of B7 III,[3] although Mandrini and Niemela (1986) suggested it may be a subgiant star with a classification of B4–5 IV.[4] The outer envelope of this star has an effective temperature of around 23,000 K, resulting in the blue-white hue of a B-type star.

The two stars have an angular separation of 5.030 arcseconds. As a binary star system, they would have an estimated orbital period of at least 19,500 years and a present-day separation of around 2,000 Astronomical Units.[4] This system is roughly 12 million years old.[6]

In the next 7500 years, the south Celestial pole will pass close to these stars and Iota Carinae (8100 CE).[10]

  1. ^ a b c d e f Cite error: The named reference aaa474_2_653 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference aass34_1 was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference mnras389_2_869 was invoked but never defined (see the help page).
  4. ^ a b c d e f g h i j k l Cite error: The named reference ikao79_57 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference mnras223_79 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  8. ^ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  9. ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 28 日 Archived 2013-05-13 at the Wayback Machine
  10. ^ "Precession".