PP Carinae
{{Short description|Star in the constellation Carina}}
{{about|p Carinae|P Carinae|V399 Carinae}}
{{Starbox begin
| name = PP Carinae
}}
{{Starbox image
| image=
{{Location mark
|image=Carina constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=12|mark_link=p Car
|x=190|y=412
}}
|caption=Location of PP Carinae (circled)
}}
{{Starbox observe
| epoch = J2000.0
| dec = {{DEC|-61|41|07.1963}}
| constell = Carina
}}
{{Starbox character
| variable = γ Cas
}}
{{Starbox astrometry
| parallax = 6.75
| p_error = 0.40
}}
{{Starbox detail
| metal_fe =
| temperature = {{val|17410|174|fmt=commas}}
| rotational_velocity = {{val|280|6}}
}}
{{Starbox catalog
| names = p Carinae, PP Carinae, CP−61°1704, FK5 397, HD 91465, HIP 51576, HR 4140, SAO 251006
}}
{{Starbox reference
|Simbad=HD+91465
}}
{{Starbox end}}
p Carinae is a star in the southern constellation of Carina. It has the variable star designation PP Carinae and, at an apparent visual magnitude of +3.3, is readily visible to the naked eye from the southern hemisphere. From the observed parallax shift of this star as the Earth orbits the Sun, its distance can be estimated as roughly {{Convert|480|ly|pc|abbr=off|lk=on}} with a 6% margin of error. It is considered to be a member of the open cluster IC 2602 although it lies well outside the core visible group of stars.
File:PPCarLightCurve.png for PP Carinae, plotted from TESS data]]
The star is a B-type main sequence star with a stellar classification of B4 Vne. The 'ne' suffix indicates it is a rapidly rotating Be star that is surrounded by hot circumstellar gas. This material adds emission lines to the spectrum of the star. It has a projected rotational velocity of {{nowrap|325 km s−1}}, with about 7.6 times the mass and eight times the radius of the Sun. Alan William James Cousins announced the discovery that this star is a variable star, in 1951. This star is classified as a Gamma Cassiopeiae-type variable and its brightness varies from magnitude +3.22 to +3.55.
In most versions of its asterism, the neighbouring bright stars, thus plotted along the imaginary hull forming Carina are Theta Carinae, to the south, and V337 (also known as lower case q) Carinae to the east, of second and third magnitude respectively.
References
{{reflist|refs=
{{cite journal | last1=Tetzlaff | first1=N. | last2=Neuhäuser | first2=R. | last3=Hohle | first3=M. M. | title=A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun | journal=Monthly Notices of the Royal Astronomical Society | volume=410 | issue=1 | pages=190–200 |date=January 2011 | doi=10.1111/j.1365-2966.2010.17434.x | doi-access=free | bibcode=2011MNRAS.410..190T |arxiv = 1007.4883 | s2cid=118629873 }}
{{cite web|url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=6067|title=VSX: Detail for PP Carinae|author=Otero, Sebastian Alberto|date=15 April 2012|work=The International Variable Star Index|publisher=American Association of Variable Star Observers|access-date=2018-01-05}}
}}
{{Stars of Carina}}
{{DEFAULTSORT:PP Carinae}}
Category:B-type main-sequence stars
Category:Carina (constellation)