This article is about h1 Puppis. For other stars with this Bayer designation, see h Puppis. For H Puppis, see HD 53811.
NS Puppis
Location of NS Puppis (circled)
Observation data Epoch J2000 Equinox J2000
Constellation
Puppis
Right ascension
08h 11m 21.4934s[1]
Declination
−39° 37′ 06.7588″[1]
Apparent magnitude (V)
4.40 - 4.50[2]
Characteristics
Evolutionary stage
Supergiant
Spectral type
K4.5 Ib[3]
Variable type
Lc[2]
Astrometry
Radial velocity (Rv)
16.20[4] km/s
Proper motion (μ)
RA: −9.072 mas/yr[1] Dec.: 3.211 mas/yr[1]
Parallax (π)
2.3831 ± 0.1188 mas[1]
Distance
1,363+62 −65 ly (418+19 −20 pc)[5]
Details
Mass
8±0.9[6]M☉
Radius
213±24[6]R☉
Luminosity
9,772[6]L☉
Surface gravity (log g)
0.73±0.02[6] cgs
Temperature
3,961±125[6] K
Other designations
h1 Pup, CD−39°4084, HD 68553, HIP 40091, HR 3225, SAO 198908
Database references
SIMBAD
data
NS Puppis (NS Pup) is an irregular variable star in the constellation Puppis. Its apparent magnitude varies between 4.4 and 4.5.
NS Puppis is a naked eye star, given the h1 and the Bright Star Catalogue number 3225. It was considered to be a stable star[8][9] until 1966.[10] It was given the variable star designation NS Puppis in 1975.[11]
h2 Puppis is another luminous K-type star with almost the same visual magnitude about a degree to the southeast.
^ abcdVallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875.
Gaia DR3 record for this source at VizieR.
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star until 1966. It was given the variable star designation NSPuppis in 1975. h2 Puppis is another luminous K-type star with almost the same visual magnitude...
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