Sigma3 Cancri

Star in the constellation Cancer


title: "Sigma3 Cancri" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["g-type-giants", "horizontal-branch-stars", "cancer-(constellation)", "bayer-objects", "bright-star-catalogue-objects", "durchmusterung-objects", "flamsteed-objects", "henry-draper-catalogue-objects", "hipparcos-objects"] description: "Star in the constellation Cancer" topic_path: "science/astronomy" source: "https://en.wikipedia.org/wiki/Sigma3_Cancri" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Star in the constellation Cancer ::

| name = Sigma3 Cancri | epoch = J2000.0 | equinox = J2000.0 (ICRS) | constell = Cancer | ra = | dec = | appmag_v = +5.24 | type = red clump | class = G9 III | b-v = +0.91 | u-b = +0.64 | r-i = | variable = | radial_v = | prop_mo_ra = −43.741 | prop_mo_dec = −34.754 | pm_footnote = | parallax = 10.7481 | p_error = 0.0965 | parallax_footnote = | absmag_v = 0.45 | source = | mass = | radius = 10.32 | luminosity = 72 | temperature = | gravity = 3.18 | metal_fe = | rotational_velocity = | age_myr = | names = | Simbad = sig03+Cnc Sigma3 Cancri is a solitary, yellow-hued star in the zodiac constellation of Cancer. Its name is a Bayer designation that is Latinized from σ3 Cancri, and abbreviated Sigma3 Cnc or σ3 Cnc. With an apparent visual magnitude of +5.24, it is a dim star that is visible to the naked eye. Based upon an annual parallax shift of as seen from Earth, it is located approximately 303 ly from the Sun. The star's proper motion makes it a candidate for membership in the IC 2391 supercluster.

This is an evolved, G-type giant star with a stellar classification of G9 III. At the estimated age of 420 million years it is a red clump star on the horizontal branch, which indicates it is generating energy through helium fusion at its core. Sigma3 Cancri has 2.8 times the mass of the Sun and has expanded to 10.3 times the Sun's radius. It is radiating 72 times the solar luminosity from its photosphere at an effective temperature of 5,170 K.

References

| 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=Reality Tests of Superclusters in the Young Disk Population | last=Eggen | first=Olin J. | journal=Astronomical Journal | postscript=. | volume=110 | page=2862 | date=December 1995 | doi=10.1086/117734 | bibcode=1995AJ....110.2862E }}

| display-authors=1 | last1=Mishenina | first1=T. V. | last2=Bienaymé | first2=O. | last3=Gorbaneva | first3=T. I. | last4=Charbonnel | first4=C. | last5=Soubiran | first5=C. | last6=Korotin | first6=S. A. | last7=Kovtyukh | first7=V. V. | title=Elemental abundances in the atmosphere of clump giants | journal=Astronomy and Astrophysics | volume=456 | issue=3 | pages=1109–1120 | date=September 2006 | doi=10.1051/0004-6361:20065141 | bibcode=2006A&A...456.1109M | arxiv=astro-ph/0605615 | s2cid=18764566 | 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=. }}

| display-authors=1 | last1=Da Silva | first1=Ronaldo | last2=Milone | first2=André de C. | last3=Rocha-Pinto | first3=Helio J. | title=Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets | journal=Astronomy & Astrophysics | postscript=. | volume=580 | pages=A24 | year=2015 | bibcode=2015A&A...580A..24D | doi=10.1051/0004-6361/201525770 | arxiv=1505.01726 | s2cid=119216425 }}

| last1=Sato | first1=K. | last2=Kuji | first2=S. | title=MK classification and photometry of stars used for time and latitude observations at Mizusawa and Washington | journal=Astronomy and Astrophysics Supplement Series | volume=85 | pages=1069 | year=1990 | bibcode=1990A&AS...85.1069S | postscript=. }}

| last1=Jofré | first1=E. | last2=Petrucci | first2=R. | last3=Saffe | first3=C. | last4=Saker | first4=L. | last5=Artur de la Villarmois | first5=E. | last6=Chavero | first6=C. | last7=Gómez | first7=M. | last8=Mauas | first8=P. J. D. | title=Stellar parameters and chemical abundances of 223 evolved stars with and without planets | journal=Astronomy & Astrophysics | display-authors=1 | volume=574 | pages=A50 | year=2015 | arxiv=1410.6422 | bibcode=2015A&A...574A..50J | doi=10.1051/0004-6361/201424474 | s2cid=53666931 | postscript=. }}

| last1=Guetter | first1=H. H. | last2=Hewitt | first2=A. V. | title=Photoelectric UBV photometry for 317 PZT and VZT stars | journal=Astronomical Society of the Pacific | volume=96 | pages=441–443 | date=1984 | postscript=. | bibcode=1984PASP...96..441G | doi=10.1086/131362 | doi-access=free }}

| title=sig03 Cnc | mode=cs2 | accessdate=2017-06-11 | postscript=. }}

References

  1. {{Cite Gaia DR3. 712117436084443008

::callout[type=info title="Wikipedia Source"] This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page. ::

g-type-giantshorizontal-branch-starscancer-(constellation)bayer-objectsbright-star-catalogue-objectsdurchmusterung-objectsflamsteed-objectshenry-draper-catalogue-objectshipparcos-objects