Pi2 Octantis
{{Short description|Star in the constellation Octans}}
{{DISPLAYTITLE:Pi2 Octantis}}
{{other stars by Bayer designation|Pi Octantis{{!}}π Octantis}}
{{Starbox begin
| name = π2 Octantis
}}
{{Starbox image
| image ={{Location mark
| image=Octans IAU.svg | alt= | float=center | width=250
| label= | position=center
| mark=Red circle.svg | mark_width=4 | mark_link=Pi2 Octantis
| x%=34 | y%=65
}}
| caption = Location of π2 Octantis (circled)
}}
{{Starbox observe
| constell = Octans
}}
{{Starbox character
}}
{{Starbox astrometry
| parallax = 2.0741
| p_error = 0.0429
}}
{{Starbox detail
| radius = {{val|69.02|1.61|1.53}}
| gravity =
| metal_fe =
| rotational_velocity = 5.7 ± 1.8
}}
{{Starbox catalog
| names = {{odlist|B = π2 Oct|Gould = 22 G. Octantis |HD = 131246|CPD = −82°636|GC = 20145|HIP = 73771|HR = 5545|SAO = 258714}}
}}
{{Starbox reference
| Simbad = pi.02+Oct
}}
{{Starbox end}}
Pi2 Octantis, Latinized from π2 Octantis, is a solitary star situated in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.64, allowing it to be faintly visible to the naked eye under ideal conditions. Located 1,570 light years away, the star is approaching the Sun with a heliocentric radial velocity of {{val|-13.8|ul=km/s}}.
This object is an ageing late G-type supergiant that has 7 times the mass of the Sun and 69.02 times the radius of the Sun. It radiates at {{val|2709|ul=solar luminosity|fmt=commas}} from its enlarged photosphere at an effective temperature of 4,588 K, giving it an orange-yellow glow. Despite its advanced state, Pi2 Octantis is still a young star at an age of 43 million years. It spins modestly with a projected rotational velocity of {{val|5.7|ul=km/s}}.
References
{{reflist||refs=
{{Cite Gaia EDR3|5771483873053059968}}
{{Cite DR2|5771483873053059968}}
{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 | s2cid=14878976 |doi-access=free}}
}}
{{Octans}}