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HD 61330

Star in the constellation Puppis From Wikipedia, the free encyclopedia

HD 61330 (f Puppis) is a binary star in the constellation Puppis. Its apparent magnitude is 4.53[3] and it is approximately 360 light years away based on parallax.[2]

Right ascension07h 37m 22.10978s[2]
Declination−34° 58 06.7109[2]
Quick facts Constellation, Right ascension ...
HD 61330
Location of HD 61330 (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Puppis[1]
Right ascension 07h 37m 22.10978s[2]
Declination −34° 58 06.7109[2]
Apparent magnitude (V) 4.53[3] + 6.87[4]
Characteristics
Evolutionary stage main sequence[5]
Spectral type B8IV[6]
U−B color index −0.31[3]
B−V color index −0.09[3]
Astrometry
Radial velocity (Rv)+24.00[7] km/s
Proper motion (μ) RA: −14.21[2] mas/yr
Dec.: +16.32[2] mas/yr
Parallax (π)9.05±0.40 mas[2]
Distance360 ± 20 ly
(110 ± 5 pc)
Absolute magnitude (MV)−0.68[1]
Orbit[8]
Period (P)78.38±2.00 yr
Semi-major axis (a)0.322±0.003
Eccentricity (e)0.655±0.005
Inclination (i)152.9±5.0°
Longitude of the node (Ω)74.7±5.0°
Periastron epoch (T)2016.754±0.500
Argument of periastron (ω)
(secondary)
208.4±5.0°
Details
f Pup A
Mass3.32±0.15[8] M
Luminosity270[5] L
Temperature11,480[5] K
Rotational velocity (v sin i)56[5] km/s
f Pup C
Mass2.11±0.10[8] M
Other designations
f Puppis, CD−34°3755, CCDM J07374-3458ABC, FK5 290, GC 10246, GSC 07113-03280, HIP 37096, HR 2937, HD 61330, SAO 198195, WDS J07374-3458AB,C
Database references
SIMBADdata
Close

The primary and secondary, with respective labels A and C, take 78 years to complete an orbit, with a considerable eccentricity of 0.655.[8] Another closer component, B, has been reported at 6.1 magnitude and 0.1" separation, but subsequent observers have repeatedly failed to confirm it.[9][10]

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