49 Cancri
{{about-distinguish|b Cancri|β Cancri}}
{{Short description|Star in the constellation Cancer}}
{{Starbox begin}}
{{Starbox image
| image=
{{Location mark
|image=Cancer constellation map.svg|alt=|float=center|width=260
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=49 Cancri
|x=480|y=720
}}
|caption=Location of 49 Cancri (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Cancer
| dec = {{DEC|+10|04|54.0073}}
}}
{{Starbox character
| type = Main sequence
| u-b =
| variable = α2 CVn
}}
{{Starbox astrometry
| parallax = 6.5062
| p_error = 0.0748
}}
{{Starbox detail
| rotation = {{val|6.907|ul=days}}
}}
{{Starbox catalog
| names = {{odlist | B=b Cnc | F=49 Cnc | V=BI Cnc | BD=+10°1864 | FK5=2688 | HD=74521 | HIP=42917 | HR=3465 | SAO=98089 }}
}}
{{Starbox reference
| Simbad = 49+Cnc
}}
{{Starbox end}}
49 Cancri is a single star in the zodiac constellation of Cancer, located 501 light years away from the Sun. It has the Bayer designation b Cancri; 49 Cancri is the Flamsteed designation. It is visible to the naked eye as a faint star with an apparent visual magnitude of about 5.6. It is moving away from the Earth with a heliocentric radial velocity of +27.5 km/s.
File:BICncLightCurve.png for BI Cancri, plotted from TESS data]]
In 1962, Helmut Abt and John C. Golson published a paper that showed that 49 Cancri was probably a variable star. It was given its variable star designation, BI Cancri, in 1962. Its brightness changes from magnitude 5.58 to 5.71 every seven days. It is classified as an α2 Canum Venaticorum variable, a class of magnetic chemically peculiar stars. The brightness changes are thought to correspond to the rotation of the star. 49 Cancri is classified from its spectrum as an Ap star, with enhanced lines of silicon, europium, and chromium. Additionally, calcium and magnesium lines are described as weaker than normal.
49 Cancri is classified as an A1 main sequence star. It has three times the mass of the Sun, an effective temperature of {{val|10615|fmt=commas|ul=K}}, and a radius of {{solar radius|2.9|link=y}}. It radiates about a hundred times the luminosity of the Sun due to its high temperature and large size.
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References
{{Reflist|refs=
{{cite simbad | title=49 Cnc | access-date=2019-07-29 }}
{{Cite Gaia DR3|598314443554350464}}
| last1=Kukarkin | first1=B. V. | last2=Kholopov | first2=P. N. | last3=Perova | first3=N. B.
| title=57th Name-List of Variable Stars | journal=Information Bulletin on Variable Stars
| date=October 1970 | volume=480 | pages=1–39 | bibcode=1970IBVS..480....1K
| url=https://articles.adsabs.harvard.edu/pdf/1970IBVS..480....1K | access-date=30 December 2024}}
| last1=Abt | first1=Helmut A. | last2=Golson | first2=John C.
| title=Colors and Variability of Magnetic Stars | journal=Astrophysical Journal
| date=July 1962 | volume=136 | pages=35–51 | doi=10.1086/147349 | bibcode=1962ApJ...136...35A
| url=https://articles.adsabs.harvard.edu/pdf/1962ApJ...136...35A | access-date=30 December 2024}}
| title=MAST: Barbara A. Mikulski Archive for Space Telescopes
| url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
| publisher=Space Telescope Science Institute | access-date=7 January 2023}}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters | arxiv=1108.4971
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | s2cid=119257644 }}
}}
{{Stars of Cancer}}
Category:A-type main-sequence stars
Category:Cancer (constellation)