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NV Puppis

NV Puppis
Puppis constellation map.svg
Red circle.svg

Location of NV Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 18m 18.39335s
Declination −36° 44′ 02.2329″
Apparent magnitude (V) 4.67
Characteristics
Spectral type B2V+B3IVne
U−B color index -0.79
B−V color index -0.10
Variable type γ Cas
Astrometry
Radial velocity (Rv) +18.60 km/s
Proper motion (μ) RA: -10.25 mas/yr
Dec.: +5.82 mas/yr
Parallax (π) 4.06 ± 0.18mas
Distance 800 ± 40 ly
(250 ± 10 pc)
Absolute magnitude (MV) -2.31
Details
Mass 10.1 M
Luminosity 12309 L
Temperature 22,000 K
Metallicity [Fe/H] 0.00 dex
Rotational velocity (v sin i) 254 km/s
Other designations
Upsilon1 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
SIMBAD data

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

It is a γ Cas variable, ranging from 4.78 to 4.58 magnitude. It is most likely an optical double with the nearby NW Puppis.

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


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