51 Camelopardalis

{{Short description|K-type giant in the constellation Camelopardalis}}

{{Starbox begin

| name = 51 Camelopardalis

}}

{{Starbox image

| image =

{{Location mark

| image = Camelopardalis constellation map.svg

| float = center | width = 260 | position = right

| mark = Red circle.svg | mark_width = 10 | mark_link = 51 Camelopardalis

| x = 181 | y = 696

}}

| caption = Location of 51 Cam on the map (circled)

}}

{{Starbox observe

| epoch = J2000.0 (ICRS)

| constell = Camelopardalis

| ra = {{RA|07|46|40.07812}}

| dec = {{DEC|+65|27|20.4266}}

| appmag_v = 5.93{{±|0.01}}

}}

{{Starbox character

| b-v = +1.18

| class = K2 III

}}

{{Starbox astrometry

| radial_v = −30.9{{±|0.2}}

| parallax = 9.7528

| p_error = 0.0372

| parallax_footnote =

| prop_mo_ra = +27.601

| prop_mo_dec = +17.656

| pm_footnote =

| absmag_v = +0.92

}}

{{Starbox detail

| mass = 1.08

| radius = 11.8{{±|0.3|0.9}}

| luminosity = 57.2{{±|0.4}}

| gravity = 2.25

| temperature = 4,626{{±|122}}

| metal_fe = +0.00

| rotational_velocity =

| age_gyr = 9.25

}}

{{Starbox catalog

| names = {{odlist|F = 51 Cam|AG = +65°409|BD = +65°593|FK5 = 2602|GC = 10420|HD = 62066|HIP = 37949|HR = 2975|SAO = 14321}}

}}

{{Starbox reference

| Simbad = 51+Cam

}}

{{Starbox end}}

51 Camelopardalis (51 Cam), also designated as HD 62066, is a solitary star located in the northern circumpolar constellation Camelopardalis. It is faintly visible to the naked eye as an orange-hued point of light with an apparent magnitude of 5.93. Gaia DR3 parallax measurements imply a distance of 334 light-years and it is currently receding with a heliocentric radial velocity of {{val|−30.9|ul=km/s}}. At its current distance, 51 Cam's brightness is diminished by 0.17 magnitudes due to interstellar extinction and it has an absolute magnitude of +0.92.

51 Cam has a stellar classification of K2 III, indicating that it is an evolved K-type giant star. It has a comparable mass to the Sun but it has more than twice the latter's age at 9.25 billion years. As a result, it has exhausted hydrogen at its core and it has expanded to 11.8 times the radius of the Sun. It radiates 57.2 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of {{val|4626|ul=K|fmt=commas}}. 51 Cam has a solar metallicity at [Fe/H] = +0.00.

References

{{reflist||refs=

{{Cite DR3|1095540363575300480}}

{{cite journal | last1 = Høg | first1 = E. | last2 = Fabricius | first2 = C. | last3 = Makarov | first3 = V. V. | last4 = Urban | first4 = S. | last5 = Corbin | first5 = T. | last6 = Wycoff | first6 = G. | last7 = Bastian | first7 = U. | last8 = Schwekendiek | first8 = P. | last9 = Wicenec | first9 = A. | title = The Tycho-2 catalogue of the 2.5 million brightest stars | journal = Astronomy and Astrophysics | date = March 2000 | volume = 355 | pages = L27–L30 | s2cid = 17128864 | bibcode = 2000A&A...355L..27H | issn = 0004-6361}}

{{cite journal | last1 = Adams | first1 = Walter S. | last2 = Joy | first2 = Alfred H. | last3 = Humason | first3 = Milton L. | last4 = Brayton | first4 = Ada Margaret | title = The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars | journal = The Astrophysical Journal | date = April 1935 | volume = 81 | page = 187 | issn = 0004-637X | eissn = 1538-4357 | doi = 10.1086/143628 | s2cid = 121056016 | bibcode = 1935ApJ....81..187A | doi-access = free}}

{{cite journal | last1=Haggkvist | first1=L. | last2=Oja | first2=T. | title=Results of BV photometry 1969-70 (Uppsala refractor) | s2cid=231475662 | journal=Private Communication | year=1970 | bibcode=1970Priv.........0H | page=}}

{{cite journal | bibcode = 2005A&A...430..165F | title = Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters | journal = Astronomy and Astrophysics | volume = 430 | pages = 165 | last1 = Famaey | first1 = B. | last2 = Jorissen | first2 = A. | last3 = Luri | first3 = X. | last4 = Mayor | first4 = M. | last5 = Udry | first5 = S. | last6 = Dejonghe | first6 = H. | last7 = Turon | first7 = C. | date = January 2005 | doi = 10.1051/0004-6361:20041272 | arxiv = astro-ph/0409579 | s2cid = 17804304 | doi-access = free}}

{{cite journal | last1 = Anderson | first1 = E. | last2 = Francis | first2 = Ch. | title = XHIP: An extended hipparcos compilation | journal = Astronomy Letters | date = May 2012 | volume = 38 | issue = 5 | pages = 331–346 | issn = 1063-7737 | eissn = 1562-6873 | doi = 10.1134/S1063773712050015 | bibcode = 2012AstL...38..331A | arxiv = 1108.4971| s2cid = 119257644}}

{{cite journal | last1 = Charbonnel | first1 = C. | last2 = Lagarde | first2 = N. | last3 = Jasniewicz | first3 = G. | last4 = North | first4 = P. L. | last5 = Shetrone | first5 = M. | last6 = Krugler Hollek | first6 = J. | last7 = Smith | first7 = V. V. | last8 = Smiljanic | first8 = R. | last9 = Palacios | first9 = A. | last10 = Ottoni | first10 = G. | title = Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era | journal = Astronomy & Astrophysics | date = January 2020 | volume = 633 | page = A34 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361/201936360 | s2cid = 204907220 | bibcode = 2020A&A...633A..34C | arxiv = 1910.12732 | doi-access = free}}

{{cite journal | display-authors = 1 | last1 = Anders | first1 = F. | last2 = Khalatyan | first2 = A. | last3 = Chiappini | first3 = C. | last4 = Queiroz | first4 = A. B. | last5 = Santiago | first5 = B. X. | last6 = Jordi | first6 = C. | last7 = Girardi | first7 = L. | last8 = Brown | first8 = A. G. A. | last9 = Matijevič | first9 = G. | last10 = Monari | first10 = G. | last11 = Cantat-Gaudin | first11 = T. | last12 = Weiler | first12 = M. | last13 = Khan | first13 = S. | last14 = Miglio | first14 = A. | last15 = Carrillo | first15 = I. | last16 = Romero-Gómez | first16 = M. | last17 = Minchev | first17 = I. | last18 = de Jong | first18 = R. S. | last19 = Antoja | first19 = T. | last20 = Ramos | first20 = P. | last21 = Steinmetz | first21 = M. | last22 = Enke | first22 = H. | title = Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18 | journal = Astronomy & Astrophysics | date = August 2019 | volume = 628 | page = A94 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361/201935765 | bibcode = 2019A&A...628A..94A | arxiv = 1904.11302 | s2cid = 131780028 | doi-access = free}}

{{Cite DR2|1095540363575300480}}

{{cite journal | display-authors = 1 | last1 = Stassun | first1 = Keivan G. | last2 = Oelkers | first2 = Ryan J. | last3 = Paegert | first3 = Martin | last4 = Torres | first4 = Guillermo | last5 = Pepper | first5 = Joshua | last6 = Lee | first6 = Nathan De | last7 = Collins | first7 = Kevin | last8 = Latham | first8 = David W. | last9 = Muirhead | first9 = Philip S. | last10 = Chittidi | first10 = Jay | last11 = Rojas-Ayala | first11 = Bárbara | last12 = Fleming | first12 = Scott W. | last13 = Rose | first13 = Mark E. | last14 = Tenenbaum | first14 = Peter | last15 = Ting | first15 = Eric B. | last16 = Kane | first16 = Stephen R. | last17 = Barclay | first17 = Thomas | last18 = Bean | first18 = Jacob L. | last19 = Brassuer | first19 = C. E. | last20 = Charbonneau | first20 = David | last21 = Ge | first21 = Jian | last22 = Lissauer | first22 = Jack J. | last23 = Mann | first23 = Andrew W. | last24 = McLean | first24 = Brian | last25 = Mullally | first25 = Susan | last26 = Narita | first26 = Norio | last27 = Plavchan | first27 = Peter | last28 = Ricker | first28 = George R. | last29 = Sasselov | first29 = Dimitar | last30 = Seager | first30 = S. | last31 = Sharma | first31 = Sanjib | last32 = Shiao | first32 = Bernie | last33 = Sozzetti | first33 = Alessandro | last34 = Stello | first34 = Dennis | last35 = Vanderspek | first35 = Roland | last36 = Wallace | first36 = Geoff | last37 = Winn | first37 = Joshua N. | title = The Revised TESS Input Catalog and Candidate Target List | journal = The Astronomical Journal | date = 9 September 2019 | volume = 158 | issue = 4 | page = 138 | eissn = 1538-3881 | doi = 10.3847/1538-3881/ab3467 | bibcode = 2019AJ....158..138S | arxiv = 1905.10694 | s2cid = 166227927 | hdl = 1721.1/124721 | hdl-access = free | doi-access = free}}

{{cite journal | last1 = Dotter | first1 = Aaron | last2 = Chaboyer | first2 = Brian | last3 = Jevremović | first3 = Darko | last4 = Kostov | first4 = Veselin | last5 = Baron | first5 = E. | last6 = Ferguson | first6 = Jason W. | title = The Dartmouth Stellar Evolution Database | journal = The Astrophysical Journal Supplement Series | s2cid = 119290835 | date = September 2008 | volume = 178 | issue = 1 | pages = 89–101 | issn = 0067-0049 | eissn = 1538-4365 | doi = 10.1086/589654 | bibcode = 2008ApJS..178...89D | arxiv = 0804.4473 | doi-access = free}}

{{Cite simbad|title = * 51 Cam|access-date = August 23, 2023}}

{{cite journal | last1 = Gontcharov | first1 = George A. | last2 = Mosenkov | first2 = Aleksandr V. | title = Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars | journal = Monthly Notices of the Royal Astronomical Society | date = 28 September 2017 | volume = 472 | issue = 4 | pages = 3805–3820 | issn = 0035-8711 | eissn = 1365-2966 | doi = 10.1093/mnras/stx2219 | bibcode = 2017MNRAS.472.3805G | arxiv = 1709.01160 | s2cid = 118879856 | doi-access = free}}

}}

{{Stars of Camelopardalis}}

Category:K-type giants

Category:Camelopardalis

Camelopardalis, 51

BD+65 00593

062066

037949

2975