Nu3 Canis Majoris
{{short description|Star in the constellation Canis Major}}
{{DISPLAYTITLE:Nu3 Canis Majoris}}
{{other stars by Bayer designation|Nu Canis Majoris{{!}}ν Canis Majoris}}
{{Starbox begin
| name = Nu3 Canis Majoris
}}
{{Starbox observe
| epoch = J2000.0
| constell = Canis Major
| dec = {{DEC|−18|14|14.9218}}
| appmag_v = 4.41 {{nowrap|(4.63 + 8.56)}}
}}
{{Starbox character
| type = horizontal branch
| variable =
}}
{{Starbox astrometry
| radial_v = {{Val|−1.50|0.70}}
| parallax = 7.74
| p_error = 0.43
}}
{{Starbox detail
| component1 = ν3 CMa A
| radius = 32.7
| luminosity = 398
| temperature = 4,510
| gravity = 2.34
| metal_fe = −0.24
| rotation = 183 d
}}
{{Starbox catalog
| names = {{odlist | B=ν3 CMa | F=8 Canis Majoris | BD=−18°1492 | FK5=| HD=47442 | HIP=31700 | HR=2443 | SAO=151730 | CCDM=06379-1814 | GC=8660 }}
}}
{{Starbox reference
| Simbad = nu03+CMa
}}
{{Starbox end}}
Nu3 Canis Majoris, Latinized from ν3 Canis Majoris, is a binary star system in the southern constellation of Canis Major.
Characteristics
The star system, appearing as one star, is deemed visible to the naked eye with its combined apparent visual magnitude of 4.41. Based upon an annual parallax shift of 7.74 mas as seen from Earth, this system is about 420 light years from the Sun, much further than Nu1 and Nu2 which appear nearby when seen from one point in the Solar System.
The primary member, component A, is an evolved, orange-hued giant/bright giant hybrid with an apparent magnitude of +4.63 and a stellar classification of K0 II-III. It is most likely (96% chance) on the horizontal branch. The star has a moderate level of surface activity with a magnetic field strength of {{Val|2.2|0.4|ul=G}} and is a source of X-ray emission with a luminosity of {{Val|624e27|u=erg s−1}}.
This giant has an estimated 3.4 times the mass of the Sun and has expanded to 33 times the Sun's radius. It is radiating 398 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,510 K. The star is spinning with the leisurely period of 183 days. Its companion, component B has been observed at 1.040 arcseconds distant and has an apparent magnitude of +8.56.
References
{{reflist|refs=
| title=Validation of the new Hipparcos reduction
| last1=van Leeuwen | first1=F.
| journal=Astronomy and Astrophysics
| volume=474 | issue=2 | pages=653–664 | date=2007
| arxiv=0708.1752 | bibcode=2007A&A...474..653V
| doi=10.1051/0004-6361:20078357 | s2cid=18759600 | postscript=. }}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015
| arxiv=1108.4971 | s2cid=119257644 | postscript=. }}
| last1=Bernacca | first1=P. L. | last2=Perinotto | first2=M.
| title=A catalogue of stellar rotational velocities
| journal=Contributi Osservatorio Astronomico di Padova in Asiago
| volume=239 | issue=1 | year=1970
| bibcode=1970CoAsi.239....1B | postscript=. }}
| 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 | doi-access=free | bibcode=2008MNRAS.389..869E
| arxiv=0806.2878 | s2cid=14878976 | postscript=. }}
| last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C.
| title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project
| journal=Astronomy & Astrophysics
| volume=546 | id=A61 | pages=14 | date=October 2012
| doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D
| arxiv=1208.3048 | s2cid=59451347 | postscript=. }}
| title=Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity
| display-authors=1 | last1=Reffert | first1=Sabine
| last2=Bergmann | first2=Christoph | last3=Quirrenbach | first3=Andreas
| last4=Trifonov | first4=Trifon | last5=Künstler | first5=Andreas
| journal=Astronomy & Astrophysics
| volume=574 | pages=A116 | year=2015
| doi=10.1051/0004-6361/201322360 | arxiv=1412.4634
| bibcode=2015A&A...574A.116R | postscript=. | hdl=10722/215277| s2cid=59334290 }}
| last1=Fernie | first1=J. D. | postscript=.
| title=New UBVRI photometry for 900 supergiants
| journal=Astrophysical Journal Supplement Series
| volume=52 | pages=7–22 | date=May 1983
| doi=10.1086/190856 | bibcode=1983ApJS...52....7F | doi-access=free }}
{{citation | display-authors=1
| title=The magnetic fields at the surface of active single G-K giants
| journal=Astronomy & Astrophysics
| last1=Aurière | first1=M. | last2=Konstantinova-Antova | first2=R.
| last3=Charbonnel | first3=C. | last4=Wade | first4=G. A.
| last5=Tsvetkova | first5=S. | last6=Petit | first6=P.
| last7=Dintrans | first7=B. | last8=Drake | first8=N. A.
| last9=Decressin | first9=T. | last10=Lagarde | first10=N.
| last11=Donati | first11=J.-F. | last12=Roudier | first12=T.
| last13=Lignières | first13=F. | last14=Schröder | first14=K.-P.
| last15=Landstreet | first15=J. D. | last16=Lèbre | first16=A.
| last17=Weiss | first17=W. W. | last18=Zahn | first18=J.-P.
| volume=574 | id=A90 | year=2015
| pages=A90
| bibcode=2015A&A...574A..90A | arxiv=1411.6230
| doi=10.1051/0004-6361/201424579 | s2cid=118504829
| postscript=. }}
| title=nu03 CMa | accessdate=2017-09-05 | postscript=. }}
}}
{{Stars of Canis Major|state=collapsed}}
{{DEFAULTSORT:Nu3 Canis Majoris}}