GJ 1062: Difference between revisions

GJ 1062
Observation data; Epoch J2000.0 Equinox J2000.0
Constellation	Eridanus
Right ascension	03h 38m 15.69799s
Declination	−11° 29′ 13.5050″
Apparent magnitude (V)	+13.010
Characteristics
Spectral type	M2.5VI
U−B color index	+1.385
B−V color index	+1.605
R−I color index	1.184
Astrometry
Radial velocity (Rv)	−84.88±0.56 km/s
Proper motion (μ)	RA: 1,458.201 mas/yr ; Dec.: −2,696.545 mas/yr
Parallax (π)	61.8861 ± 0.0220 mas
Distance	52.70 ± 0.02 ly ; (16.159 ± 0.006 pc)
Absolute magnitude (MV)	10.608
Details
Mass	0.255 M☉
Radius	0.411±0.051 R☉; 0.372±0.076 R☉; 0.202±0.012 R☉
Luminosity	0.0055 L☉
Temperature	3,488±50 K
Metallicity [Fe/H]	−0.28±0.15 dex
Rotational velocity (v sin i)	9.80 km/s
Other designations
	GJ 1062, LHS 20, LTT 1717, Ross 578, 2MASS J03381558-1129102
Database references
SIMBAD	data
ARICNS	data

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GJ 1062 is a single^[6] red dwarf star in the constellation Eridanus, positioned about two degrees to the SSE of Epsilon Eridani.^[9] It is also known as LHS 20 and Ross 578. The star is invisible to the naked eye with an apparent visual magnitude of +13.0,^[2] requiring a telescope with at least a 25 cm (10 in) aperture to view.^[10] It is located at a distance of 52.7 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −85 km/s.^[1] The star has a high proper motion, traversing the sky at the rate of 3.033 arcseconds per year.^[11]

This is an M-type subdwarf star with a stellar classification of M2.5VI.^[3] It was one of the first three subdwarfs to be definitively identified by G. Kuiper in 1940, the other two being Kapteyn's Star and Wolf 1106.^[12] GJ 1062 is considered a likely member of the halo population, and thus is a MACHO.^[13]

References

^ ^a ^b ^c ^d ^e ^f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
^ ^a ^b ^c ^d ^e ^f ^g Houdebine, E. R. (2010). "Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars". Monthly Notices of the Royal Astronomical Society. 407 (3): 1657. Bibcode:2010MNRAS.407.1657H. doi:10.1111/j.1365-2966.2010.16827.x.
^ ^a ^b Gizis, John E. (1997). "M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale". Astronomical Journal. 113: 806–822. arXiv:astro-ph/9611222. Bibcode:1997AJ....113..806G. doi:10.1086/118302. S2CID 16863021.
^ ^a ^b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
^ ^a ^b Houdebine, E. R.; et al. (May 2016). "Rotation-Activity Correlations in K and M Dwarfs. I. Stellar Parameters and Compilations of v sin I and P/sin I for a Large Sample of Late-K and M Dwarfs". The Astrophysical Journal. 822 (2): 38. arXiv:1604.07920. Bibcode:2016ApJ...822...97H. doi:10.3847/0004-637X/822/2/97. S2CID 119118088. 97.
^ ^a ^b Winters, Jennifer G.; et al. (June 2019). "The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc". The Astronomical Journal. 157 (6): 32. arXiv:1901.06364. Bibcode:2019AJ....157..216W. doi:10.3847/1538-3881/ab05dc. S2CID 86859146. 216.
^ ^a ^b Kesseli, Aurora Y.; et al. (February 2019). "Radii of 88 M Subdwarfs and Updated Radius Relations for Low-metallicity M-dwarf Stars". The Astronomical Journal. 157 (2): 17. arXiv:1810.07702. Bibcode:2019AJ....157...63K. doi:10.3847/1538-3881/aae982. S2CID 119325209. 63.
^ "GJ 1062". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 December 2016.
^ Sinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. Vol. 1. Sky Publishing Corporation and the European Space Agency. p. 308. ISBN 0-933346-84-0.
^ "The astronomical magnitude scale". International Comet Quarterly. Retrieved 2020-12-31.
^ Luyten, W. J. (June 1995). "NLTT Catalogue". VizieR Online Data Catalog. Bibcode:1995yCat.1098....0L.
^ Kotoneva, E.; et al. (August 2005). "A study of Kapteyn's star". Astronomy and Astrophysics. 438 (3): 957–962. Bibcode:2005A&A...438..957K. doi:10.1051/0004-6361:20042287.
^ Fuchs, B.; Jahreiß, H. (January 1998). "Halo stars in the immediate solar neighbourhood". Astronomy and Astrophysics. 329: 81. arXiv:astro-ph/9708209. Bibcode:1998A&A...329...81F.

[GaiaDR3-1] ^ ^a ^b ^c ^d ^e ^f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.

[Houdebine2010-2] ^ ^a ^b ^c ^d ^e ^f ^g Houdebine, E. R. (2010). "Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars". Monthly Notices of the Royal Astronomical Society. 407 (3): 1657. Bibcode:2010MNRAS.407.1657H. doi:10.1111/j.1365-2966.2010.16827.x.

[Gizis1977-3] Gizis, John E. (1997). "M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale". Astronomical Journal. 113: 806–822. arXiv:astro-ph/9611222. Bibcode:1997AJ....113..806G. doi:10.1086/118302. S2CID 16863021.

[UBV-4] Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.

[Houdebine_et_al_2016-5] Houdebine, E. R.; et al. (May 2016). "Rotation-Activity Correlations in K and M Dwarfs. I. Stellar Parameters and Compilations of v sin I and P/sin I for a Large Sample of Late-K and M Dwarfs". The Astrophysical Journal. 822 (2): 38. arXiv:1604.07920. Bibcode:2016ApJ...822...97H. doi:10.3847/0004-637X/822/2/97. S2CID 119118088. 97.

[Winters_et_al_2019-6] Winters, Jennifer G.; et al. (June 2019). "The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc". The Astronomical Journal. 157 (6): 32. arXiv:1901.06364. Bibcode:2019AJ....157..216W. doi:10.3847/1538-3881/ab05dc. S2CID 86859146. 216.

[Kesseli_et_al_2019-7] Kesseli, Aurora Y.; et al. (February 2019). "Radii of 88 M Subdwarfs and Updated Radius Relations for Low-metallicity M-dwarf Stars". The Astronomical Journal. 157 (2): 17. arXiv:1810.07702. Bibcode:2019AJ....157...63K. doi:10.3847/1538-3881/aae982. S2CID 119325209. 63.

[SIMBAD-8] "GJ 1062". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 December 2016.

[Sinnott_Perryman_1997-9] Sinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. Vol. 1. Sky Publishing Corporation and the European Space Agency. p. 308. ISBN 0-933346-84-0.

[ICQ-10] "The astronomical magnitude scale". International Comet Quarterly. Retrieved 2020-12-31.

[Luyten1995-11] Luyten, W. J. (June 1995). "NLTT Catalogue". VizieR Online Data Catalog. Bibcode:1995yCat.1098....0L.

[Kotoneva_et_al_2005-12] Kotoneva, E.; et al. (August 2005). "A study of Kapteyn's star". Astronomy and Astrophysics. 438 (3): 957–962. Bibcode:2005A&A...438..957K. doi:10.1051/0004-6361:20042287.

[Fuchs_Jahreiß_1998-13] Fuchs, B.; Jahreiß, H. (January 1998). "Halo stars in the immediate solar neighbourhood". Astronomy and Astrophysics. 329: 81. arXiv:astro-ph/9708209. Bibcode:1998A&A...329...81F.

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@@ Line 1: / Line 1: @@
+{{Short description|Star in the constellation Eridanus}}
-{{Starbox begin
+{{Starbox begin}}
-| name = Gliese 1062
-}}
 {{Starbox observe
-| epoch = [[J2000.0]]
+ | epoch       = [[J2000.0]]
-| constell = [[Eridanus (constellation)|Eridanus]]
+ | constell    = [[Eridanus (constellation)|Eridanus]]
-| ra = {{RA|03|38|15.580}}<ref name="SIMBAD">{{cite simbad | title=GJ 1062 | access-date=4 December 2016}}</ref>
+ | ra          = {{RA|03|38|15.69799}}<ref name=GaiaDR3/>
-| dec = {{DEC|-11|29|10.29}}<ref name="SIMBAD"/>
+ | dec         = {{DEC|−11|29|13.5050}}<ref name=GaiaDR3/>
-| appmag_v = +13.02<ref name="SIMBAD"/>
+ | appmag_v    = +13.010<ref name=Houdebine2010/>
 }}
 {{Starbox character
+ | type        =
-| class = M2.5VI<ref>{{cite journal|author1=Gizis, John E. |date=1997|title=M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale |journal=Astronomical Journal|volume=113|pages=806–822|url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=1997AJ....113..806G|bibcode=1997AJ....113..806G|doi=10.1086/118302|arxiv=astro-ph/9611222|s2cid=16863021}}</ref>
-| b-v = +1.605<ref name=UBV>{{cite journal
+ | class       = M2.5VI<ref name=Gizis1977/>
+ | b-v         = +1.605<ref name=UBV/>
-    | author1=Mermilliod, J.-C.
+ | u-b         = +1.385<ref name=UBV />
-    | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)
+ | r-i         = 1.184<ref name=Houdebine2010/>
-    | journal=Catalogue of Eggen's UBV Data
+ | variable    =
- | url = http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?1986EgUBV........0M&db_key=AST&nosetcookie=1
-    | date=1986
-    | bibcode= 1986EgUBV........0M }}</ref>
-| u-b = +1.385<ref name=UBV />
 }}
 {{Starbox astrometry
-| radial_v=-104.3<ref name="SIMBAD" />
+ | radial_v    = {{val|−84.88|0.56}}<ref name=GaiaDR3/>
-| prop_mo_ra=1461<ref name="SIMBAD" />
+ | prop_mo_ra  = {{val|1458.201|fmt=commas}}
-| prop_mo_dec=-2699<ref name="SIMBAD" />
+ | prop_mo_dec = {{val|−2696.545|fmt=commas}}
+ | pm_footnote = <ref name=GaiaDR3/>
-|parallax=62.4
+ | parallax    = 61.8861
-|p_error=3.30
+ | p_error     = 0.0220
-| parallax_footnote=<ref>{{cite journal|author1=Jao, Wei-Chun|display-authors=etal|date=2011|title=The Solar Neighborhood. XXIV. Parallax Results from the CTIOPI 0.9 m Program: Stars with μ ≥ 1farcs0 yr-1 (MOTION Sample) and Subdwarfs|journal=The Astronomical Journal|volume=141|issue=4|pages=117–127|bibcode=2011AJ....141..117J|doi=10.1088/0004-6256/141/4/117|arxiv=1102.0994|s2cid=118723387}}</ref>
-| absmag_v=12.0<ref name=ARICNS/>
+ | parallax_footnote = <ref name=GaiaDR3/>
+ | absmag_v    = 10.608<ref name=Houdebine_et_al_2016/>
 }}
 {{Starbox detail
+ | mass        = 0.255<ref name=Winters_et_al_2019/>
-|radius=0.202<ref name=dM1>{{cite journal|author1=Houdebine, E. R. |date=2010|title=Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars |journal=Monthly Notices of the Royal Astronomical Society|volume=407|issue=3|page=1657|url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2010MNRAS.407.1657H|bibcode=2010MNRAS.407.1657H|doi=10.1111/j.1365-2966.2010.16827.x|doi-access=free}}</ref>
+ | radius      = {{val|0.411|0.051|u=solar radius}}<ref name=Houdebine2010/><br>{{val|0.372|0.076|u=solar radius}}<ref name=Houdebine_et_al_2016/><br>{{val|0.202|0.012}}<ref name=Kesseli_et_al_2019/>
-|temperature=3488<ref name=dM1/>
+ | luminosity  = 0.0055<ref name=Houdebine2010/>
-|
+ | temperature = {{val|3488|50|fmt=commas}}<ref name=Houdebine2010/>
+ | gravity     =
+ | metal_fe    = {{val|−0.28|0.15}}<ref name=Kesseli_et_al_2019/>
+ | rotational_velocity = 9.80<ref name=Houdebine2010/>
+ | age_gyr     =
 }}
 {{Starbox catalog
-| names=[[Gliese Catalogue of Nearby Stars|Gliese]] 1062, [[Luyten Half-Second catalogue|LHS]] 20, [[Luyten Two-Tenths catalogue|LTT]] 1717, [[Ross catalogue|Ross]] 578, [[2MASS]] J03381558-1129102
+ | names = {{odlist | GJ=1062 | LHS=20 | LTT=1717 | Ross=578 | 2MASS=J03381558-1129102 }}<ref name="SIMBAD"/>
 }}
 {{Starbox reference
-| Simbad = GJ+1062
+ | Simbad = GJ+1062
-| ARICNS = 02025
+ | ARICNS = 02025
 }}
 {{Starbox end}}
-'''Gliese 1062''' is a [[M-type star|M-type]] [[subdwarf]] [[star]] in the [[constellation]] [[Eridanus (constellation)|Eridanus]].<ref name="ARICNS">{{cite web|work=University of Heidelberg|url=http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c02025.htm|title=ARICNS ARI Data Base for Nearby Stars|access-date=31 July 2012}}</ref>
-<ref>{{citation|last=Bakich|first=Michael E.|title=The Cambridge Guide to the Constellations|url=https://books.google.com/books?id=tLMXiFhTnRYC&pg=PA95|year=1995|publisher=Cambridge University Press|isbn=978-0-521-44921-2|page=95}}</ref>
-The star has a total [[proper motion]] of 3.033 [[Minute of arc#Astronomy|"]]/[[year|yr]], making it the 25th-fastest-moving star in terms of angular position as seen from Earth, and its [[radial velocity]] is -18 [[kilometres per second|km/s]]. At a [[Distance measures (cosmology)|distance]] of about 52 [[light year]]s (16 [[parsec]]s) and with an [[absolute magnitude]] of 13.1, this star has an [[apparent magnitude]] of 14.6 when viewed from [[Earth]].<ref>[http://csep10.phys.utk.edu/astr162/lect/motion/table.html University of Tennessee Department of Physics and Astronomy, Table:Proper Motion: Stars with very large proper motion. accessdate = 31 July 2012]</ref><ref>Martin V. Zombeck ''Handbook of Space Astronomy And Astrophysics'' Cambridge University Press. 2007 page 86.</ref>
+'''GJ 1062''' is a single<ref name=Winters_et_al_2019/> [[red dwarf]] [[star]] in the [[constellation]] [[Eridanus (constellation)|Eridanus]], positioned about two degrees to the SSE of [[Epsilon Eridani]].<ref name=Sinnott_Perryman_1997/> It is also known as [[Luyten Half-Second catalogue|LHS]] 20 and [[Frank Elmore Ross|Ross]] 578. The star is invisible to the naked eye with an [[apparent visual magnitude]] of +13.0,<ref name=Houdebine2010/> requiring a telescope with at least a {{convert|25|cm|in|0|abbr=on}} [[aperture]] to view.<ref name=ICQ/> It is located at a distance of 52.7&nbsp;[[light year]]s from the [[Sun]] based on [[stellar parallax|parallax]], but is drifting closer with a [[radial velocity]] of −85&nbsp;km/s.<ref name=GaiaDR3/> The star has a high [[proper motion]], traversing the sky at the rate of {{val|3.033|ul=arcseconds}} per year.<ref name=Luyten1995/>
-The star is also known as [[Luyten Half-Second catalogue|LHS]] 20 and [[Frank Elmore Ross|Ross]] 578.
+This is an [[M-type star|M-type]] [[subdwarf]] star with a [[stellar classification]] of M2.5VI.<ref name=Gizis1977/> It was one of the first three subdwarfs to be definitively identified by [[Gerard Kuiper|G. Kuiper]] in 1940, the other two being [[Kapteyn's Star]] and [[Wolf 1106]].<ref name=Kotoneva_et_al_2005/> GJ 1062 is considered a likely member of the [[galactic halo|halo]] population, and thus is a [[MACHO]].<ref name=Fuchs_Jahreiß_1998/>
 == References ==
-{{reflist}}
+{{reflist|refs=
+<ref name=GaiaDR3>{{Cite Gaia DR3|5115463180914712448}}</ref>
+<ref name="SIMBAD">{{cite simbad | title=GJ 1062 | access-date=4 December 2016}}</ref>
+<ref name=Houdebine_et_al_2016>{{cite journal
+ | title=Rotation-Activity Correlations in K and M Dwarfs. I. Stellar Parameters and Compilations of v sin I and P/sin I for a Large Sample of Late-K and M Dwarfs
+ | last1=Houdebine | first1=E. R. | last2=Mullan | first2=D. J.
+ | last3=Paletou | first3=F. | last4=Gebran | first4=M.
+ | display-authors=1 | journal=The Astrophysical Journal
+ | volume=822 | issue=2 | id=97 | pages=38 | date=May 2016
+ | arxiv=1604.07920 | bibcode=2016ApJ...822...97H
+ | doi=10.3847/0004-637X/822/2/97 | s2cid=119118088 | doi-access=free }}</ref>
+<ref name=Luyten1995>{{cite journal
+ | journal=VizieR Online Data Catalog
+ | title=NLTT Catalogue | date=June 1995
+ | last=Luyten | first=W. J.
+ | bibcode=1995yCat.1098....0L }}</ref>
+<ref name=Sinnott_Perryman_1997>{{cite book
+ | first1=Roger W. | last1=Sinnott
+ | first2=Michael A. C. | last2=Perryman
+ | title=Millennium Star Atlas | page=308
+ | volume=1 | year=1997 | isbn=0-933346-84-0
+ | publisher=Sky Publishing Corporation and the European Space Agency }}</ref>
+<ref name=ICQ>{{cite web
+ | title=The astronomical magnitude scale
+ | work=International Comet Quarterly
+ | url=http://www.icq.eps.harvard.edu/MagScale.html
+ | access-date=2020-12-31 }}</ref>
+<ref name=Fuchs_Jahreiß_1998>{{cite journal
+ | title=Halo stars in the immediate solar neighbourhood
+ | last1=Fuchs | first1=B. | last2=Jahreiß | first2=H.
+ | journal=Astronomy and Astrophysics | volume=329 | page=81 | date=January 1998
+ | arxiv=astro-ph/9708209 | bibcode=1998A&A...329...81F }}</ref>
+<ref name=Winters_et_al_2019>{{cite journal
+ | title=The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc
+ | display-authors=1 | last1=Winters | first1=Jennifer G.
+ | last2=Henry | first2=Todd J. | last3=Jao | first3=Wei-Chun
+ | last4=Subasavage | first4=John P. | last5=Chatelain | first5=Joseph P.
+ | last6=Slatten | first6=Ken | last7=Riedel | first7=Adric R.
+ | last8=Silverstein | first8=Michele L. | last9=Payne | first9=Matthew J.
+ | journal=The Astronomical Journal
+ | volume=157 | issue=6 | id=216 | pages=32 | date=June 2019
+ | arxiv=1901.06364 | bibcode=2019AJ....157..216W
+ | doi=10.3847/1538-3881/ab05dc | s2cid=86859146 | doi-access=free }}</ref>
+<ref name=Gizis1977>{{cite journal
+ | last=Gizis | first=John E.
+ | title=M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale
+ | journal=Astronomical Journal
+ | volume=113 | pages=806–822 | date=1997
+ | doi=10.1086/118302 | arxiv=astro-ph/9611222
+ | bibcode=1997AJ....113..806G | s2cid=16863021 }}</ref>
+<ref name=UBV>{{cite journal
+ | last=Mermilliod | first=J.-C.
+ | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)
+ | journal=Catalogue of Eggen's UBV Data
+ | date=1986 | bibcode= 1986EgUBV........0M
+ | url = http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?1986EgUBV........0M&db_key=AST&nosetcookie=1 }}</ref>
+<ref name=Houdebine2010>{{cite journal
+ | last=Houdebine | first=E. R.
+ | title=Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars
+ | journal=Monthly Notices of the Royal Astronomical Society
+ | volume=407 | issue=3 | page=1657 | date=2010
+ | doi=10.1111/j.1365-2966.2010.16827.x | doi-access=free
+ | bibcode=2010MNRAS.407.1657H }}</ref>
+<ref name=Kesseli_et_al_2019>{{cite journal
+ | title=Radii of 88 M Subdwarfs and Updated Radius Relations for Low-metallicity M-dwarf Stars
+ | last1=Kesseli | first1=Aurora Y. | last2=Kirkpatrick | first2=J. Davy
+ | last3=Fajardo-Acosta | first3=Sergio B. | last4=Penny | first4=Matthew T.
+ | last5=Gaudi | first5=B. Scott | last6=Veyette | first6=Mark
+ | last7=Boeshaar | first7=Patricia C. | last8=Henderson | first8=Calen B.
+ | last9=Cushing | first9=Michael C. | last10=Calchi-Novati | first10=Sebastiano
+ | last11=Shvartzvald | first11=Y. | last12=Muirhead | first12=Philip S.
+ | display-authors=1 | journal=The Astronomical Journal
+ | volume=157 | issue=2 | id=63 | pages=17 | date=February 2019
+ | arxiv=1810.07702 | bibcode=2019AJ....157...63K
+ | doi=10.3847/1538-3881/aae982 | s2cid=119325209 | doi-access=free }}</ref>
+<ref name=Kotoneva_et_al_2005>{{cite journal
+ | title=A study of Kapteyn's star
+ | display-authors=1 | last1=Kotoneva | first1=E.
+ | last2=Innanen | first2=K. | last3=Dawson | first3=P. C.
+ | last4=Wood | first4=P. R. | last5=De Robertis | first5=M. M.
+ | journal=Astronomy and Astrophysics
+ | volume=438 | issue=3 | date=August 2005 | pages=957–962
+ | doi=10.1051/0004-6361:20042287 | bibcode=2005A&A...438..957K | doi-access=free }}</ref>
+}}
 {{Stars of Eridanus}}
@@ Line 56: / Line 154: @@
 [[Category:Eridanus (constellation)]]
 [[Category:Gliese and GJ objects|1062]]
-[[Category:2MASS objects]]
+[[Category:Ross objects|578]]
+[[Category:2MASS objects|J03381558-1129102]]
+[[Category:TIC objects|38403917]]
-{{reddwarf-star-stub}}

Observation data Epoch J2000.0 Equinox J2000.0
Constellation	Eridanus
Right ascension	03^h 38^m 15.69799^s^[1]
Declination	−11° 29′ 13.5050″^[1]
Apparent magnitude (V)	+13.010^[2]
Characteristics
Spectral type	M2.5VI^[3]
U−B color index	+1.385^[4]
B−V color index	+1.605^[4]
R−I color index	1.184^[2]
Astrometry

Radial velocity (R_v)	−84.88±0.56^[1] km/s
Proper motion (μ)	RA: 1,458.201 mas/yr^[1] Dec.: −2,696.545 mas/yr^[1]
Parallax (π)	61.8861 ± 0.0220 mas^[1]
Distance	52.70 ± 0.02 ly (16.159 ± 0.006 pc)
Absolute magnitude (M_V)	10.608^[5]

Details

Mass	0.255^[6] `M`_☉
Radius	0.411±0.051 R_☉^[2] 0.372±0.076 R_☉^[5] 0.202±0.012^[7] `R`_☉
Luminosity	0.0055^[2] `L`_☉
Temperature	3,488±50^[2] K
Metallicity [Fe/H]	−0.28±0.15^[7] dex
Rotational velocity (v sin i)	9.80^[2] km/s

Other designations
GJ 1062, LHS 20, LTT 1717, Ross 578, 2MASS J03381558-1129102^[8]
Database references
SIMBAD	data
ARICNS	data