List of nearest giant stars

{{Short description|none}}

This is a list of the nearest giant stars (luminosity class III or II) to the Earth, located at a distance of up to {{Convert|100|ly|pc}}.

List

{{Sticky header}}

class="wikitable sortable sticky-header"

!Name

!{{nowrap|Distance (ly)}}

!{{nowrap|Spectral type}}

!{{nowrap|Stellar radius}} ({{Solar radius}})

!{{nowrap|Stellar mass}} ({{Solar mass}})

!Apparent magnitude (V)

!Notes

Pollux

|{{val|33.78|0.09}}

|style="background: {{star-color|K}};"| K0 III{{Cite journal |last1=Morgan |first1=W. W. |last2=Keenan |first2=P. C. |date=1973-01-01 |title=Spectral Classification |url=https://ui.adsabs.harvard.edu/abs/1973ARA&A..11...29M |journal=Annual Review of Astronomy and Astrophysics |volume=11 |pages=29–50 |doi=10.1146/annurev.aa.11.090173.000333 |bibcode=1973ARA&A..11...29M |issn=0066-4146}}

|{{ntsh|8.97}}{{Val|8.97|0.03}}

|{{ntsh|1.91}}{{Val|1.91|0.09}}

|1.14

|17th brightest star in the night sky and the nearest red giant/red clump.

Arcturus

|{{val|36.7|0.2}}

|style="background: {{star-color|K}};"|{{nowrap|K1.5 III Fe−0.5}}{{Cite web |title=alf Boo |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=HD+124897 |access-date=2023-12-22 |website=SIMBAD}}

|{{ntsh|25.4}}{{Val|25.4|0.2}}

|{{ntsh|1.08}}{{Val|1.08|0.06}}

| -0.05

|Fourth-brightest star in the night sky, and the nearest red-giant branch star to Earth.

Capella A

|rowspan="2"| {{val|42.919|0.049}}

|style="background: {{star-color|G}};"|G8III

|{{ntsh|11.98}}{{nowrap|11.98 ± 0.57}}

|{{ntsh|2.569}}{{val|2.569|0.007}}

|0.03

|The nearest yellow giant, together with Capella A. With a magnitude of 0.08,{{Cite book |last1=Hoffleit |first1=Dorrit |url=https://ui.adsabs.harvard.edu/abs/1991bsc..book.....H |title=The Bright star catalogue |last2=Jaschek |first2=Carlos |date=1991-01-01|bibcode=1991bsc..book.....H}} the Capella star system is the 6th-brightest star in the night sky.

Capella B

|style="background: {{star-color|G}};"|G0III

|{{ntsh|8.83}}{{nowrap|8.83 ± 0.33}}

|{{ntsh|2.483}}{{val|2.483|0.007}}

|0.16

|The nearest yellow giant, together with Capella B.

Errai {{Nowrap|(Gamma Cephei A)}}

|{{val|44.98|0.09}}{{cite DR3|2281778105594488192}}

|style="background: {{star-color|K}};"|K1III-IVCN1{{Cite web |title=Gamma Cephei |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=Gamma+Cephei |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|4.74}}{{val|4.74|0.03|0.08}}

|{{ntsh|1.27}}{{val|1.27|0.05|0.07}}

|3.21{{Cite journal |last1=Hoffleit |first1=D. |last2=Warren |first2=W. H. Jr. |date=1995-11-01 |title=VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) |url=https://ui.adsabs.harvard.edu/abs/1995yCat.5050....0H |journal=VizieR Online Data Catalog |pages=V/50|bibcode=1995yCat.5050....0H}}

|

Caph {{Nowrap|(Beta Cassiopeiae)}}

|{{val|54.7|0.3}}

|style="background: {{star-color|F}};"|F2 III{{Cite web |title=beta Cas |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=beta+Cas |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|3.69}}{{nowrap|3.69 × 3.43}}

|{{ntsh|1.91}}1.91 ± 0.02

|2.28 {{nowrap|(2.25–2.31)}}{{Cite journal |last1=Kukarkin |first1=B. V. |last2=Kholopov |first2=P. N. |last3=Pskovsky |first3=Y. P. |last4=Efremov |first4=Y. N. |last5=Kukarkina |first5=N. P. |last6=Kurochkin |first6=N. E. |last7=Medvedeva |first7=G. I. |date=1971-01-01 |title=The third edition containing information on 20437 variable stars discovered and designated till 1968. |url=https://ui.adsabs.harvard.edu/abs/1971GCVS3.C......0K |journal=General Catalogue of Variable Stars |pages=0|bibcode=1971GCVS3.C......0K}}

|{{nowrap|The nearest F-type giant.}}

Chi Eridani

|{{val|57.3|0.2}}{{cite DR3|4937200425857908992 }}

|style="background: {{star-color|G}};"|G8IIIb CNIV

|{{val|4.0|0.03}}

|1.58

|3.70{{Cite journal |last=Mermilliod |first=J. -C. |date=1986-01-01 |title=Compilation of Eggen's UBV data, transformed to UBV (unpublished) |url=https://ui.adsabs.harvard.edu/abs/1986EgUBV........0M |journal=Catalogue of Eggen's UBV Data |pages=0|bibcode=1986EgUBV........0M}}

|

Menkent (Theta Centauri)

|{{val|58.8|0.2}}

|style="background: {{star-color|K}};"|K0 III{{Cite journal |last1=Gray |first1=R. O. |last2=Corbally |first2=C. J. |last3=Garrison |first3=R. F. |last4=McFadden |first4=M. T. |last5=Bubar |first5=E. J. |last6=McGahee |first6=C. E. |last7=O'Donoghue |first7=A. A. |last8=Knox |first8=E. R. |date=July 2006 |title=Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample |journal=The Astronomical Journal |volume=132 |issue=1 |pages=161–170 |doi=10.1086/504637 |arxiv=astro-ph/0603770 |bibcode=2006AJ....132..161G |issn=0004-6256}}

|{{ntsh|10.77}}{{val|10.77|0.45}}{{cite journal |last1=Fuhrmann |first1=K. |last2=Chini |first2=R. |date=2012 |title=Multiplicity among F-type Stars |journal=The Astrophysical Journal Supplement |volume=203 |issue=2 |pages=20 |bibcode=2012ApJS..203...30F |doi=10.1088/0067-0049/203/2/30 |id=30 =|doi-access=free}}

|{{ntsh|1.27}}1.27{{Cite journal |last1=Halbwachs |first1=Jean-Louis |last2=Mayor |first2=Michel |last3=Udry |first3=Stéphane |date=November 2018 |title=Multiplicity among solar-type stars IV. The CORAVEL radial velocities and the spectroscopic orbits of nearby K dwarfs |journal=Astronomy & Astrophysics |volume=619 |pages=A81 |doi=10.1051/0004-6361/201833377 |arxiv=1808.04605 |bibcode=2018A&A...619A..81H |issn=0004-6361}}

|2.06

|

Epsilon Reticuli

|{{val|60.1|0.1}}{{cite DR3|4678664766393829504}}

|style="background: {{star-color|K}};"|K2III-IV

|{{ntsh|3.18}}{{val|3.18|0.08}}

|{{ntsh|1.46}}{{val|1.46|0.01}}

|4.44

|

Eta Serpentis

|{{val|60.5|0.2}}

|style="background: {{star-color|K}};"|K0III-IV{{Cite web |title=eta Ser |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=eta+Ser |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|5.897}}5.897 ± 0.028{{Cite journal |last1=Mérand |first1=A. |last2=Kervella |first2=P. |last3=Barban |first3=C. |last4=Josselin |first4=E. |last5=ten Brummelaar |first5=T. A. |last6=McAlister |first6=H. A. |last7=Coudé du Foresto |first7=V. |last8=Ridgway |first8=S. T. |last9=Turner |first9=N. |last10=Sturmann |first10=J. |last11=Sturmann |first11=L. |last12=Goldfinger |first12=P. J. |last13=Farrington |first13=C. |date=2010-07-01 |title=Interferometric radius and limb darkening of the asteroseismic red giant η Serpentis with the CHARA Array |journal=Astronomy and Astrophysics |volume=517 |pages=A64 |doi=10.1051/0004-6361/200912103 |bibcode=2010A&A...517A..64M |issn=0004-6361|doi-access=free}}

|{{ntsh|1.7}}{{val|1.7|0.3}}{{Cite journal |last=Lagarde |first=N. |last2=Miglio |first2=A. |last3=Eggenberger |first3=P. |last4=Morel |first4=T. |last5=Montalbán |first5=J. |last6=Mosser |first6=B. |last7=Rodrigues |first7=T. S. |last8=Girardi |first8=L. |last9=Rainer |first9=M. |last10=Poretti |first10=E. |last11=Barban |first11=C. |last12=Hekker |first12=S. |last13=Kallinger |first13=T. |last14=Valentini |first14=M. |last15=Carrier |first15=F. |date=August 2015 |title=Models of red giants in the CoRoT asteroseismology fields combining asteroseismic and spectroscopic constraints |url=http://www.aanda.org/10.1051/0004-6361/201525856 |journal=Astronomy & Astrophysics |volume=580 |pages=A141 |doi=10.1051/0004-6361/201525856 |issn=0004-6361|arxiv=1505.01529 }}

|3.26

|

Alpha Trianguli (Mothallah)

|{{val|63.3|0.3}}

|style="background: {{star-color|F}};"|F5III{{Cite web |title=alf Tri |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=alf+Tri |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|3.22}}3.22

|{{ntsh|1.7}}1.7

|3.42

|

Tureis (Rho Puppis)

|{{val|63.5|0.2}}

|style="background: {{star-color|F}};"|F5IIkF2IImF5II{{Cite web |title=rho Pup |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=rho+Pup |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|3.52}}{{Val|3.52|0.07}}

|{{ntsh|1.5}}{{Val|1.5|0.1}}

|2.78{{Cite journal |last1=Bookmeyer |first1=B. B. |last2=Fitch |first2=W. S. |last3=Lee |first3=T. A. |last4=Wisniewski |first4=W. Z. |last5=Johnson |first5=H. L. |date=1977-08-01 |title=Photoelectric UBV observations of RR Lyrae variable stars. Second list. |url=https://ui.adsabs.harvard.edu/abs/1977RMxAA...2..235B |journal=Revista Mexicana de Astronomía y Astrofísica |volume=2 |pages=235–258 |bibcode=1977RMxAA...2..235B |issn=0185-1101}} {{nowrap|(2.68 – 2.87)}}{{Cite journal |last1=Samus' |first1=N. N. |last2=Kazarovets |first2=E. V. |last3=Durlevich |first3=O. V. |last4=Kireeva |first4=N. N. |last5=Pastukhova |first5=E. N. |date=2017-01-01 |title=General catalogue of variable stars: Version GCVS 5.1 |url=https://ui.adsabs.harvard.edu/abs/2017ARep...61...80S |journal=Astronomy Reports |volume=61 |issue=1 |pages=80–88 |doi=10.1134/S1063772917010085 |bibcode=2017ARep...61...80S |s2cid=255195566 |issn=1063-7729}}

|{{nowrap|The nearest bright giant.}}

Larawag (Epsilon Scorpii)

|{{val|63.7|0.3}}

|style="background: {{star-color|K}};"|K1 III{{Cite web |title=eps Sco |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=eps+Sco |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|12.6}}12.6{{Efn|Calculated using an angular diameter of 5.99 mas.|name=Angular diameter Larawag}}

|{{ntsh|1.24}}1.24{{Cite journal |last1=Fuhrmann |first1=K. |last2=Chini |first2=R. |last3=Kaderhandt |first3=L. |last4=Chen |first4=Z. |date=2017-02-01 |title=Multiplicity among Solar-type Stars |journal=The Astrophysical Journal |volume=836 |issue=1 |pages=139 |doi=10.3847/1538-4357/836/1/139 |bibcode=2017ApJ...836..139F |issn=0004-637X |doi-access=free}}

|2.31{{Cite journal |last1=Gutierrez-Moreno |first1=Adelina |last2=Moreno |first2=Hugo |date=1968-06-01 |title=A Photometric Investigation of the SCORPlO-CENTAURUS Association |journal=The Astrophysical Journal Supplement Series |volume=15 |pages=459 |doi=10.1086/190168 |bibcode=1968ApJS...15..459G |issn=0067-0049|doi-access=free}} {{nowrap|(2.24 – 2.35)}}

|

Nu2 Canis Majoris

|{{val|64.4|0.3}}{{Cite journal |last1=Gaia Collaboration |last2=Brown |first2=A. G. A. |last3=Vallenari |first3=A. |last4=Prusti |first4=T. |last5=de Bruijne |first5=J. H. J. |last6=Babusiaux |first6=C. |last7=Bailer-Jones |first7=C. A. L. |date=August 2018 |title=Gaia Data Release 2. Summary of the contents and survey properties |journal=Astronomy & Astrophysics |volume=616 |pages=A1 |doi=10.1051/0004-6361/201833051 |arxiv=1804.09365 |bibcode=2018A&A...616A...1G |issn=0004-6361}}

|style="background: {{star-color|K}};"|K1.5III-IVFe1{{Cite web |title=7 CMa |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=7+CMa |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|5.198}}{{Val|5.198|0.060}}{{Citation |last=Lin |first=Wen-Xu |title=Using Asteroseismology to Calibrate the Physical Parameters of Confirmed Exoplanets and Their Evolved Host Stars |date=2024-07-01 |journal=The Astronomical Journal |volume=168 |issue=1 |pages=27 |arxiv=2405.15162 |bibcode=2024AJ....168...27L |doi=10.3847/1538-3881/ad4ffc |issn=0004-6256 |last2=Qian |first2=Sheng-Bang |last3=Zhu |first3=Li-Ying |last4=Liao |first4=Wen-Ping |last5=Li |first5=Fu-Xing |doi-access=free}}

|{{ntsh|1.439}}{{Val|1.439|0.047}}

|3.96{{Cite journal |last1=Setiawan |first1=J. |last2=Pasquini |first2=L. |last3=da Silva |first3=L. |last4=Hatzes |first4=A. P. |last5=von der Lühe |first5=O. |last6=Girardi |first6=L. |last7=de Medeiros |first7=J. R. |last8=Guenther |first8=E. |date=2004-07-01 |title=Precise radial velocity measurements of G and K giants. Multiple systems and variability trend along the Red Giant Branch |journal=Astronomy and Astrophysics |volume=421 |pages=241–254 |doi=10.1051/0004-6361:20041042-1 |bibcode=2004A&A...421..241S |issn=0004-6361|doi-access=free}}

|

Aldebaran

|{{val|65.3|1}}{{Cite journal |last=Gatewood |first=George |date=2008-06-13 |title=Astrometric Studies of Aldebaran, Arcturus, Vega, the Hyades, and Other Regions |journal=The Astronomical Journal |volume=136 |issue=1 |pages=452–460 |doi=10.1088/0004-6256/136/1/452 |bibcode=2008AJ....136..452G |issn=0004-6256|doi-access=free}}

|style="background: {{star-color|K}};"|K5+III{{Cite web |title=* alf Tau |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=HD+29139 |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|45.1}} 45.1 ± 0.1{{Cite journal |last1=Hatzes |first1=A. P. |last2=Cochran |first2=W. D. |last3=Endl |first3=M. |last4=Guenther |first4=E. W. |last5=MacQueen |first5=P. |last6=Hartmann |first6=M. |last7=Zechmeister |first7=M. |last8=Han |first8=I. |last9=Lee |first9=B.-C. |last10=Walker |first10=G. A. H. |last11=Yang |first11=S. |last12=Larson |first12=A. M. |last13=Kim |first13=K.-M. |last14=Mkrtichian |first14=D. E. |last15=Doellinger |first15=M. |date=August 2015 |title=Long-lived, long-period radial velocity variations in Aldebaran: A planetary companion and stellar activity |journal=Astronomy & Astrophysics |volume=580 |pages=A31 |doi=10.1051/0004-6361/201425519 |arxiv=1505.03454 |bibcode=2015A&A...580A..31H |issn=0004-6361}}

|{{ntsh|1.16}}1.16 ± 0.07{{Cite journal |last1=Farr |first1=Will M. |last2=Pope |first2=Benjamin J. S. |last3=Davies |first3=Guy R. |last4=North |first4=Thomas S. H. |last5=White |first5=Timothy R. |last6=Barrett |first6=Jim W. |last7=Miglio |first7=Andrea |last8=Lund |first8=Mikkel N. |last9=Antoci |first9=Victoria |last10=Andersen |first10=Mads Fredslund |last11=Grundahl |first11=Frank |last12=Huber |first12=Daniel |date=2018-09-27 |title=Aldebaran b's Temperate Past Uncovered in Planet Search Data |journal=The Astrophysical Journal |volume=865 |issue=2 |pages=L20 |doi=10.3847/2041-8213/aadfde |arxiv=1802.09812 |bibcode=2018ApJ...865L..20F |issn=2041-8213 |doi-access=free}}

|0.86 {{nowrap|(0.75 – 0.95)}}{{Cite web |title=GCVS Query forms |url=http://www.sai.msu.su/gcvs/cgi-bin/search.cgi?search=alf+Tau |access-date=2023-12-22|website=www.sai.msu.su}}

|14th brightest star in the night sky.

Hamal

|{{val|65.8|0.3}}

|style="background: {{star-color|K}};"|K2-IIIbCa-1{{Cite web |title=alf Ari |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=alf+ari |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|15.19}}{{val|15.19|0.10}}

|{{ntsh|1.5}}{{val|1.5|0.2}}{{Cite journal |last1=Lee |first1=B.-C. |last2=Mkrtichian |first2=D. E. |last3=Han |first3=I. |last4=Kim |first4=K.-M. |last5=Park |first5=M.-G. |date=May 2011 |title=A likely exoplanet orbiting the oscillating K-giant Alpha Arietis |journal=Astronomy & Astrophysics |volume=529 |pages=A134 |doi=10.1051/0004-6361/201016293 |arxiv=1104.4431 |bibcode=2011A&A...529A.134L |issn=0004-6361}}

|2.00

|49th brightest star in the night sky.

Alpha Serpentis

|{{Val|74.0|0.3}}

| style="background: {{star-color|K}};" |K2IIIbCN1{{Cite web |title=alf Ser|url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=alf+Ser |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|12.19}}12.19

|{{ntsh|1.61}}1.61

|2.623

|

Epsilon Cygni

|{{Val|72.7|0.2}}

|style="background: {{star-color|K}};"|K0III{{Cite web |title=* eps Cyg |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=HD+197989 |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|11.18}}11.18

|{{ntsh|1.103}}{{val|1.103|0.042}}{{Citation |last=Heeren |first=Paul |title=Precise radial velocities of giant stars - XV. Mysterious nearly periodic radial velocity variations in the eccentric binary ε Cygni |date=2021-03-01 |journal=Astronomy & Astrophysics |volume=647 |pages=A160 |language=en |arxiv=2102.01999 |bibcode=2021A&A...647A.160H |doi=10.1051/0004-6361/202040087 |issn=0004-6361 |last2=Reffert |first2=Sabine |last3=Trifonov |first3=Trifon |last4=Wong |first4=Ka Ho |last5=Lee |first5=Man Hoi |last6=Lillo-Box |first6=Jorge |last7=Quirrenbach |first7=Andreas |last8=Arentoft |first8=Torben |last9=Albrecht |first9=Simon |last10=Grundahl |first10=Frank |last11=Andersen |first11=Mads Fredslund |last12=Antoci |first12=Victoria |last13=Pallé |first13=Pere L.}}

|2.48

|

Kaus Borealis (Lambda Sagittarii)

|{{val|78.2|0.3}}

|style="background: {{star-color|K}};"|K1IIIb{{Cite web |title=lam Sgr |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=lam+Sgr |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|12.692}}{{val|12.692|0.181}}

|{{ntsh|1.79}}{{val|1.79|0.20}}

|2.82{{Cite journal |last1=Wielen |first1=R. |last2=Schwan |first2=H. |last3=Dettbarn |first3=C. |last4=Lenhardt |first4=H. |last5=Jahreiß |first5=H. |last6=Jährling |first6=R. |date=1999-01-01 |title=Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions. |url=https://ui.adsabs.harvard.edu/abs/1999VeARI..35....1W |journal=Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg |volume=35 |pages=1|bibcode=1999VeARI..35....1W}}

|

Cebalrai (Beta Ophiuchi)

|{{val|81.8|0.3}}

|style="background: {{star-color|K}};"|K2IIICN0.5{{Cite web |title=bet Oph |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=bet+Oph |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|12.17}}{{val|12.17|0.06}}

|{{ntsh|1.75}}{{val|1.75|0.14}}{{Cite journal |last=Soubiran |first=C. |last2=Creevey |first2=O. L. |last3=Lagarde |first3=N. |last4=Brouillet |first4=N. |last5=Jofré |first5=P. |last6=Casamiquela |first6=L. |last7=Heiter |first7=U. |last8=Aguilera-Gómez |first8=C. |last9=Vitali |first9=S. |last10=Worley |first10=C. |last11=de Brito Silva |first11=D. |date=2024-02-01 |title=Gaia FGK benchmark stars: Fundamental Teff and log g of the third version |url=https://ui.adsabs.harvard.edu/abs/2024A&A...682A.145S |journal=Astronomy and Astrophysics |volume=682 |pages=A145 |doi=10.1051/0004-6361/202347136 |issn=0004-6361}}

|2.749

|

Alioth

|{{val|82.6|0.4}}

|style="background: {{star-color|A}};"|A1III-IVpkB9{{Cite web |title=ALIOTH |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=ALIOTH |access-date=December 22, 2023 |website=SIMBAD}}

|{{ntsh|4.29}}{{val|4.29|0.19|0.21}}

|{{ntsh|2.91}}2.91{{Cite journal |last1=Shaya |first1=Ed |last2=Olling |first2=Rob |date=2011-01-01 |title=Very Wide Binaries and Other Comoving Stellar Companions: A Bayesian Analysis of the Hipparcos Catalogue |journal=The Astrophysical Journal Supplement Series |volume=192 |issue=1 |pages=2 |doi=10.1088/0067-0049/192/1/2 |arxiv=1007.0425 |bibcode=2011ApJS..192....2S |issn=0067-0049}}

|1.77

|33rd brightest star in the night sky.

Ankaa (Alpha Phoenicis)

|{{val|85}}

|style="background: {{star-color|K}};"|K0.5IIIb{{Cite web |title=alf Phe |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=alf+Phe |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|14.7}}14.7{{Efn|Calculated using an angular diameter of 5.25 mas.|name=Angular diameter Ankaa}}

|{{ntsh|2.79}}2.79 ± 0.14{{Cite journal |last1=Kervella |first1=Pierre |last2=Arenou |first2=Frédéric |last3=Thévenin |first3=Frédéric |date=2022-01-01 |title=Stellar and substellar companions from Gaia EDR3. Proper-motion anomaly and resolved common proper-motion pairs |bibcode=2022A&A...657A...7K |journal=Astronomy and Astrophysics |volume=657 |pages=A7 |doi=10.1051/0004-6361/202142146 |arxiv=2109.10912 |issn=0004-6361}}

|2.377

|

Seginus (Gamma Boötis)

|{{val|86.8|0.3}}

|style="background: {{star-color|A}};"|A7 III{{Cite journal |last1=Ventura |first1=R. |last2=Catanzaro |first2=G. |last3=Christensen-Dalsgaard |first3=J. |last4=Di Mauro |first4=M. P. |last5=Paterno' |first5=L. |date=2007-11-11 |title=A spectroscopic search for non-radial pulsations in the delta Scuti star gamma Bootis |journal=Monthly Notices of the Royal Astronomical Society |volume=381 |issue=4 |pages=1647–1654 |doi=10.1111/j.1365-2966.2007.12334.x |doi-access=free |arxiv=0708.2364 |bibcode=2007MNRAS.381.1647V |issn=0035-8711}} or A7 IV+(n){{Cite journal |last1=Gray |first1=R. O. |last2=Napier |first2=M. G. |last3=Winkler |first3=L. I. |date=2001-04-01 |title=The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars |url=https://iopscience.iop.org/article/10.1086/319956/meta |journal=The Astronomical Journal |language=en |volume=121 |issue=4 |pages=2148 |doi=10.1086/319956 |bibcode=2001AJ....121.2148G |s2cid=117076031 |issn=1538-3881|url-access=subscription }}

|{{ntsh|4.65}}4.65

|{{nts|2.1}}{{Cite journal |last1=De Rosa |first1=R. J. |last2=Patience |first2=J. |last3=Wilson |first3=P. A. |last4=Schneider |first4=A. |last5=Wiktorowicz |first5=S. J. |last6=Vigan |first6=A. |last7=Marois |first7=C. |last8=Song |first8=I. |last9=Macintosh |first9=B. |last10=Graham |first10=J. R. |last11=Doyon |first11=R. |last12=Bessell |first12=M. S. |last13=Thomas |first13=S. |last14=Lai |first14=O. |date=2014-01-01 |title=The VAST Survey - III. The multiplicity of A-type stars within 75 pc |journal=Monthly Notices of the Royal Astronomical Society |volume=437 |issue=2 |pages=1216–1240 |doi=10.1093/mnras/stt1932 |doi-access=free |arxiv=1311.7141 |bibcode=2014MNRAS.437.1216D |issn=0035-8711}}

|3.03{{Cite journal |last1=Gray |first1=R. O. |last2=Napier |first2=M. G. |last3=Winkler |first3=L. I. |date=April 2001 |title=The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars |url=https://doi.org/10.1086/319956 |journal=The Astronomical Journal |volume=121 |issue=4 |pages=2148–2158 |doi=10.1086/319956 |bibcode=2001AJ....121.2148G |s2cid=117076031 |issn=0004-6256|url-access=subscription }} {{nowrap|(3.02 – 3.07)}}

|

Wazn (Beta Columbae)

|{{val|87.2|0.3}}

|style="background: {{star-color|K}};"|K1III_CN+1{{Cite web |title=bet Col |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=bet+col |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|11.5}}11.5{{Efn|Calculated using an angular diameter of 3.99 mas.|name=Angular diameter Wazn}}

|{{ntsh|1.1}}{{val|1.1|0.2}}

|3.105

|

Gacrux

|{{val|88.6|0.4}}

|style="background: {{star-color|M}};"|M3.5III{{Cite simbad |title=Gamma Crucis|access-date=December 22, 2023}}

|{{ntsh|73}}73{{Cite journal |last1=Nielsen |first1=Krister E. |last2=Airapetian |first2=Vladimir S. |last3=Carpenter |first3=Kenneth G. |last4=Rau |first4=Gioia |date=2023-08-01 |title=The Advanced Spectral Library: The Evolution of Chromospheric Wind Characteristics from Noncoronal to Hybrid Giant Stars |journal=The Astrophysical Journal |volume=953 |issue=1 |pages=16 |doi=10.3847/1538-4357/acdcf1 |doi-access=free |bibcode=2023ApJ...953...16N |issn=0004-637X}}

|{{ntsh|1.5}}{{val|1.5|0.3}}{{Cite journal |last1=Kallinger |first1=T. |last2=Beck |first2=P. G. |last3=Hekker |first3=S. |last4=Huber |first4=D. |last5=Kuschnig |first5=R. |last6=Rockenbauer |first6=M. |last7=Winter |first7=P. M. |last8=Weiss |first8=W. W. |last9=Handler |first9=G. |last10=Moffat |first10=A. F. J. |last11=Pigulski |first11=A. |last12=Popowicz |first12=A. |last13=Wade |first13=G. A. |last14=Zwintz |first14=K. |date=2019-04-01 |title=Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation |url=https://www.aanda.org/articles/aa/abs/2019/04/aa34514-18/aa34514-18.html |journal=Astronomy & Astrophysics |language=en |volume=624 |pages=A35 |doi=10.1051/0004-6361/201834514 |arxiv=1902.07531 |bibcode=2019A&A...624A..35K |issn=0004-6361}}

|1.64

|The nearest M-type red giant, and the 25th brightest star in the night sky.

36 G. Doradus

|{{val|89.1|0.2}}

|style="background: {{star-color|K}};"|K2III-IV

|{{ntsh|4.76}}{{val|4.76|0.14}}

|{{ntsh|1.28}}{{val|1.28|0.03}}{{Citation |last1=Malla |first1=Sai Prathyusha |last2=Stello |first2=Dennis |last3=Montet |first3=Benjamin T |last4=Huber |first4=Daniel |last5=Hon |first5=Marc |last6=Bedding |first6=Timothy R |last7=Reyes |first7=Claudia |last8=Hey |first8=Daniel R |date=2024-11-01 |title=Benchmarking the spectroscopic masses of 249 evolved stars using asteroseismology with TESS |journal=Monthly Notices of the Royal Astronomical Society |volume=534 |issue=3 |pages=1775–1786 |bibcode=2024MNRAS.534.1775M |doi=10.1093/mnras/stae2179 |doi-access=free |arxiv=2409.11736 |issn=0035-8711}}

|4.66

|

Cursa (Beta Eridani)

|{{val|90|0.9}}

|style="background: {{star-color|A}};"|A3 III var{{Cite journal |last1=Royer |first1=F. |last2=Grenier |first2=S. |last3=Baylac |first3=M.-O. |last4=Gomez |first4=A. E. |last5=Zorec |first5=J. |date=October 2002 |title=Rotational velocities of A-type stars II. Measurement of vsini in the northern hemisphere |journal=Astronomy & Astrophysics |volume=393 |issue=3 |pages=897–911 |doi=10.1051/0004-6361:20020943 |arxiv=astro-ph/0205255 |issn=0004-6361}} or A3 IV{{Cite web |title=bet Eri |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=bet+Eri |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|2.4}}{{Val|3.14|0.18}}

|{{ntsh|2.55}}2.55

|2.796

|

Delta Muscae

|{{Val|91|1}}

|style="background: {{star-color|K}};"|K2 III

|{{ntsh|8.6}}8.6

|{{ntsh|1.5}}1.5

|3.61

|

Kappa Ophiuchi

|{{val|91.5|0.5}}

|style="background: {{star-color|K}};"|K2III{{Cite web |title=kap Oph |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=kap+Oph |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|11}}11{{Cite journal |last1=Massarotti |first1=Alessandro |last2=Latham |first2=David W. |last3=Stefanik |first3=Robert P. |last4=Fogel |first4=Jeffrey |date=2008-01-01 |title=Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity |journal=The Astronomical Journal |volume=135 |issue=1 |pages=209–231 |doi=10.1088/0004-6256/135/1/209 |bibcode=2008AJ....135..209M |issn=0004-6256|doi-access=free}}

|{{ntsh|1.19}}1.19 ± 0.14

|3.20{{Cite journal |last1=Jennens |first1=P. A. |last2=Helfer |first2=H. L. |date=1975-09-01 |title=A new photometric metal abundance and luminosity calibration for field G and K giants. |journal=Monthly Notices of the Royal Astronomical Society |volume=172 |issue=3 |pages=667–679 |doi=10.1093/mnras/172.3.667 |bibcode=1975MNRAS.172..667J |issn=0035-8711|doi-access=free}}

|

Eta Draconis

|{{val|92.1|0.2}}

|style="background: {{star-color|G}};"|G8 III{{Cite web |title=eta Dra |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=eta+Dra |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|10.46}}10.46–10.53

|{{ntsh|2.55}}{{val|2.55|0.26}}{{Citation |last1=Rosas-Portilla |first1=F. |last2=Schröder |first2=K.-P. |last3=Jack |first3=D. |date=2022-04-26 |title=On the physical nature of the Wilson-Bappu effect: revising the gravity and temperature dependence |arxiv=2203.16593 |journal=Monthly Notices of the Royal Astronomical Society |volume=513 |issue=1 |pages=906–924 |doi=10.1093/mnras/stac929 |doi-access=free |issn=0035-8711}}

|2.73{{Cite journal |last1=Takeda |first1=Yoichi |last2=Sato |first2=Bun'ei |last3=Murata |first3=Daisuke |date=2008-08-25 |title=Stellar Parameters and Elemental Abundances of Late-G Giants |journal=Publications of the Astronomical Society of Japan |volume=60 |issue=4 |pages=781–802 |doi=10.1093/pasj/60.4.781 |arxiv=0805.2434 |issn=0004-6264}}

|

37 Librae

|{{Val|94.3|0.6}}

|style="background: {{star-color|K}};"|K1III-IV

|{{Ntsh|5.133}}{{VAL|5.133|0.043}}

|{{Ntsh|1.38}}{{VAL|1.38|0.1}}

|4.62{{cite simbad|title=37 Lib}}

|

|

Praecipua (46 Leonis Minoris)

|{{val|94.9|0.6}}

|style="background: {{star-color|K}};"|K0+III-IV{{Cite web |title=46 LMi|url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=46+LMi |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|8.21}}{{Val|8.21|0.05}}

|{{ntsh|1.09}}{{Val|1.09|0.04}}{{Cite journal |last=Frandsen |first=S. |last2=Andersen |first2=M. Fredslund |last3=Brogaard |first3=K. |last4=Jiang |first4=C. |last5=Arentoft |first5=T. |last6=Grundahl |first6=F. |last7=Kjeldsen |first7=H. |last8=Christensen-Dalsgaard |first8=J. |last9=Weiss |first9=E. |last10=Pallé |first10=P. |last11=Antoci |first11=V. |last12=Kjærgaard |first12=P. |last13=Sørensen |first13=A. N. |last14=Skottfelt |first14=J. |last15=Jørgensen |first15=U. G. |date=2018-05-01 |title=The mass and age of the first SONG target: the red giant 46 LMi |url=https://www.aanda.org/articles/aa/abs/2018/05/aa30816-17/aa30816-17.html |journal=Astronomy & Astrophysics |language=en |volume=613 |pages=A53 |doi=10.1051/0004-6361/201730816 |issn=0004-6361|arxiv=1806.02095}}

|3.83{{Cite journal |last1=Piau |first1=L. |last2=Kervella |first2=P. |last3=Dib |first3=S. |last4=Hauschildt |first4=P. |date=February 2011 |title=Surface convection and red giants radii measurements |journal=Astronomy & Astrophysics |volume=526 |pages=A100 |doi=10.1051/0004-6361/201014442 |arxiv=1010.3649 |bibcode=2011A&A...526A.100P |issn=0004-6361}} {{nowrap|(3.79 – 3.84)}}

|

Diphda (Beta Ceti)

|{{val|96.3|0.5}}

|style="background: {{star-color|K}};"|K0 III{{Cite journal |last1=Montes |first1=D. |last2=Lopez-Santiago |first2=J. |last3=Galvez |first3=M. C. |last4=Fernandez-Figueroa |first4=M. J. |last5=De Castro |first5=E. |last6=Cornide |first6=M. |date=November 2001 |title=Late-type stars members of young stellar kinematic groups - I. Single stars |journal=Monthly Notices of the Royal Astronomical Society |volume=328 |issue=1 |pages=45–63 |doi=10.1046/j.1365-8711.2001.04781.x|doi-access=free |arxiv=astro-ph/0106537 |bibcode=2001MNRAS.328...45M}}

|{{ntsh|17.5}}{{val|17.5|0.9}}{{cite journal|bibcode=2013MNRAS.434..437C|arxiv=1306.3288|title=Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER|journal=Monthly Notices of the Royal Astronomical Society|volume=434|pages=437|last1=Cruzalèbes|first1=P.|last2=Jorissen|first2=A.|last3=Rabbia|first3=Y.|last4=Sacuto|first4=S.|last5=Chiavassa|first5=A.|last6=Pasquato|first6=E.|last7=Plez|first7=B.|last8=Eriksson|first8=K.|last9=Spang|first9=A.|last10=Chesneau|first10=O.|year=2013|issue=1|doi=10.1093/mnras/stt1037|doi-access=free |s2cid=49573767}}

|{{ntsh|3.5}}3.5{{Cite journal |last=Tsvetkova |first=S. |last2=Petit |first2=P. |last3=Aurière |first3=M. |last4=Konstantinova-Antova |first4=R. |last5=Wade |first5=G. A. |last6=Charbonnel |first6=C. |last7=Decressin |first7=T. |last8=Bogdanovski |first8=R. |date=2013-08-01 |title=Magnetic field structure in single late-type giants: β Ceti in 2010–2012 |url=https://www.aanda.org/articles/aa/abs/2013/08/aa21051-13/aa21051-13.html |journal=Astronomy & Astrophysics |language=en |volume=556 |pages=A43 |doi=10.1051/0004-6361/201321051 |issn=0004-6361|arxiv=1301.1592}}

|2.02

|

Altais (Delta Draconis)

|{{val|97.4|0.3}}

|style="background: {{star-color|G}};"|G9III{{Cite web |title=del Dra |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=del+Dra |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|10.52}}{{Val|10.52|0.24}}

|{{ntsh|1.7}}{{val|1.70|0.18}}

|3.07

|

Alpha Indi

|{{val|99.1|0.7}}{{Cite DR3|6674382927491854848}}

|style="background: {{star-color|K}};"|K0III-IV{{Cite web |title=alf Ind |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=alf%20Ind |access-date=December 23, 2023 |website=SIMBAD}}

|{{ntsh|9.89}}{{val|9.89|0.21}}

|{{ntsh|2.15}}{{val|2.15|0.13}}

|3.11

|

Notes and references

{{reflist|refs=

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{{Cite journal |last1=Ottoni |first1=G. |last2=Udry |first2=S. |last3=Ségransan |first3=D. |last4=Buldgen |first4=G. |last5=Lovis |first5=C. |last6=Eggenberger |first6=P. |last7=Pezzotti |first7=C. |last8=Adibekyan |first8=V. |last9=Marmier |first9=M. |last10=Mayor |first10=M. |last11=Santos |first11=N. C. |last12=Sousa |first12=S. G. |last13=Lagarde |first13=N. |last14=Charbonnel |first14=C. |date=2022-01-01 |title=CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars |bibcode=2022A&A...657A..87O |journal=Astronomy and Astrophysics |volume=657 |pages=A87 |doi=10.1051/0004-6361/202040078 |issn=0004-6361|arxiv=2201.01528}} Note: Parameters are in [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/657/A87 VizieR tables].

{{Cite journal |last=van Leeuwen |first=F. |date=November 2007 |title=Validation of the new Hipparcos reduction |journal=Astronomy & Astrophysics |volume=474 |issue=2 |pages=653–664 |doi=10.1051/0004-6361:20078357 |arxiv=0708.1752 |bibcode=2007A&A...474..653V |issn=0004-6361}}

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{{DEFAULTSORT:Nearest giant stars}}

Category:Giant stars

Category:Lists of stars