Delta3 Canis Minoris
{{Short description|Star in the constellation Canis Minor}}
{{DISPLAYTITLE:Delta3 Canis Minoris}}
{{other stars by Bayer designation|Delta Canis Minoris{{!}}δ Canis Minoris}}
{{Starbox begin
| name=δ3 Canis Minoris
}}
{{Starbox image
| image=
{{Location mark
|image=Canis Minor constellation map.svg|alt=|float=center|width=220
|label=|position=right
|mark=Red circle.svg|mark_width=8|mark_link=δ3 Canis Minoris
|x=460|y=806
}}
|caption=Location of δ3 Canis Minoris (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Canis Minor
| dec = {{DEC|+03|22|18.1956}}
}}
{{Starbox character
| variable =
}}
{{Starbox astrometry
| parallax = 4.4602
| p_error = 0.1061
| parallax_footnote = {{cite DR2|203136371800297365632}}
}}
{{Starbox detail
| source =
| gravity =
| metal_fe =
}}
{{Starbox catalog
| names = {{odlist | B=δ3 CMi | F=9 CMi | BD=+03°1719 | HD=60357 | HIP=36812 | HR=2901 | SAO=115644 | GC=10128 | CCDM=07343+0322 }}
}}
{{Starbox reference
| Simbad = del03+CMi
}}
{{Starbox end}}
Delta3 Canis Minoris, Latinized from δ3 Canis Minoris, is a solitary, white-hued star in the equatorial constellation of Canis Minor. Based upon a parallax of {{val|4.46|ul=mas}} as seen from Gaia spacecraft in its repeated orbits around the Sun, just beyond the Earth. This star is about 730 light years from the Solar System. At that distance, the visual magnitude of these stars is diminished by an extinction of more than 0.15 due to interstellar dust. With an apparent visual magnitude of +5.81, it is just bright enough to be faintly visible to the naked eye.
This is a B-type main-sequence star with a stellar classification of B9 V. It is about {{Val|93.7|2.9|u=%}} of the way through its main sequence lifetime and is spinning rapidly with a projected rotational velocity of 259 km/s. The star has an estimated 3.16 times the mass of the Sun and about 2.1 times the Sun's radius. It is radiating 175 times the Sun's luminosity from its photosphere at an effective temperature of 9,908 K.
References
{{reflist|refs=
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{{citation | display-authors=1
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| arxiv=0806.2878 | s2cid=14878976 | postscript=. }}
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| journal=Astronomy & Astrophysics
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| arxiv=1208.3048 | s2cid=59451347 | postscript=. }}
| title=Rotational velocities of A-type stars. IV. Evolution of rotational velocities
| journal=Astronomy & Astrophysics
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| volume=537 | pages=A120 | year=2012
| doi=10.1051/0004-6361/201117691 | bibcode=2012A&A...537A.120Z
| arxiv=1201.2052 | s2cid=55586789
| postscript=. }}
| title=Michigan catalogue of two-dimensional spectral types for the HD Stars
| last1=Houk | first1=N. | last2=Swift | first2=C.
| journal=Michigan Spectral Survey
| volume=5 | year=1999 | postscript=.
| bibcode=1999MSS...C05....0H }}
| title=Ubvrijkl Photometry of the Bright Stars
| journal=Communications of the Lunar and Planetary Laboratory
| last1=Johnson | first1=H. L. | last2=Mitchell | first2=R. I.
| last3=Iriarte | first3=B. | last4=Wisniewski | first4=W. Z.
| year=1966 | volume=4 | pages=99
|bibcode=1966CoLPL...4...99J | postscript=. }}
| title=del03 CMi | access-date=2017-09-03 | postscript=. }}
}}
{{Stars of Canis Minor|state=collapsed}}
{{DEFAULTSORT:Delta3 Canis Minoris}}
Category:B-type main-sequence stars