NV Puppis

Star in the constellation Puppis From Wikipedia, the free encyclopedia

NV Puppis (NV Pup), also known as υ1 Puppis, is a class B2V[3] (blue main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.67[2] and it is approximately 800 light years away based on parallax.[1]

A light curve for NV Puppis, plotted from Hipparcos data[13]
Right ascension07h 18m 18.39335s[1]
Declination−36° 44 02.2329[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
NV Puppis
Location of NV Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 18m 18.39335s[1]
Declination −36° 44 02.2329[1]
Apparent magnitude (V) 4.67[2]
Characteristics
Spectral type B2V+B3IVne[3]
U−B color index −0.79[2]
B−V color index −0.10[2]
Variable type γ Cas[4]
Astrometry
Radial velocity (Rv)+18.60[5] km/s
Proper motion (μ) RA: −10.25[1] mas/yr
Dec.: +5.82[1] mas/yr
Parallax (π)4.06±0.18 mas[1]
Distance800 ± 40 ly
(250 ± 10 pc)
Absolute magnitude (MV)−2.31[6]
Details
Mass10.1[7] M
Radius8.4[8] R
Luminosity12,300[9] L
Surface gravity (log g)4.00[8] cgs
Temperature24,380[10] K
Metallicity [Fe/H]0.00[11] dex
Rotation0.466 days[10]
Rotational velocity (v sin i)254[12] km/s
Other designations
Upsilon1 Puppis, Upsilon1 Pup, υ1 Puppis, υ1 Pup, NV Puppis, NV Pup, CD−36°3512, CCDM J07184-3645A, GC 9733, GSC 07115-03016, HIP 35363, HR 2787, HD 57150, SAO 197824, WDS J07183-3644A
Database references
SIMBADdata
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It is a γ Cas variable, ranging from 4.78 to 4.58 magnitude.[4] It is most likely an optical double with the nearby NW Puppis.[14]

Neither component of this double is given a letter in Lacaille's catalogue or the British Association star catalogue.[15][16] Gould gave them the designations (Latin letter) v1 and v2 Puppis, but these are rarely used.[17] Lacaille applied the Greek letter υ to the star now called υ Carinae.[15] The designation υ1 first appeared in several catalogues at the end of the 19th century.[18]

References

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