GJ 1005
{{Short description|Star system in the constellation Cetus}}
{{Sky|00|15|28.11090|−|16|08|01.6303|19.58}}
{{Starbox begin|name=GJ 1005}}
{{Starbox observe
|epoch=J2000
|constell=Cetus
}}
{{Starbox character
}}
{{Starbox astrometry
|parallax=166.6
|p_error=0.3
|absmag_v=12.70 ± 0.01 / 15.12 ± 0.09
}}
{{Starbox orbit
|period_unitless=4.55726{{±|0.00075|0.00074}} y.{{citation|arxiv=1811.06938|year=2019|title=How to Constrain Your M Dwarf. II. The Mass–Luminosity–Metallicity Relation from 0.075 to 0.70 Solar Masses|doi=10.3847/1538-4357/aaf3bc|last1=Mann|first1=Andrew W.|last2=Dupuy|first2=Trent|last3=Kraus|first3=Adam L.|last4=Gaidos|first4=Eric|last5=Ansdell|first5=Megan|last6=Ireland|first6=Michael|last7=Rizzuto|first7=Aaron C.|last8=Hung|first8=Chao-Ling|last9=Dittmann|first9=Jason|last10=Factor|first10=Samuel|last11=Feiden|first11=Gregory|last12=Martinez|first12=Raquel A.|last13=Ruíz-Rodríguez|first13=Dary|last14=Chia Thao|first14=Pa|journal=The Astrophysical Journal|volume=871|issue=1 |page=63|bibcode=2019ApJ...871...63M |s2cid=119372932 |doi-access=free }}
|axis=0.3037 ± 0.0005
|inclination=143.93{{±|0.25|0.24}}
|node=62.8 ± 0.4
|periastron=JD 2449850.4 ± 0.8
|eccentricity=0.36136{{±|0.00097|0.00098}}
|periarg=166.6 ± 0.5
}}
{{Starbox detail
|component1=GJ 1005 A
|mass=0.179 ± 0.002
|component2=GJ 1005 B
|mass2=0.112 ± 0.001
}}
{{Starbox catalog
|names={{odlist|G=158-50|G2=266-76|HIP=1242|LHS=1047|LP=764-87|LTT=114|2MASS=J00152799-1608008|Gaia DR2=2368293487260807040}}
}}
{{Starbox reference
|Simbad=G+158-50
|ARICNS=01957|an=A
|ARICNS2=01958|an2=B
}}
{{Starbox image
|image={{Location map|100x100|AlternativeMap=Cetus_constellation_map.svg
|alt=GJ 1005 is located in the constellation Cetus.
|caption=Location of GJ 1005 in the constellation Cetus|border=infobox|mark=Red_pog.png|width=300
|label=GJ 1005
|position=top
|lat=27.3
|long=88.5
}}|caption=
}}
{{Starbox end}}
GJ 1005 is a system of two red dwarfs, located in constellation Cetus at 19.6 light-years from Earth.{{r|Hershey}} The primary star is a M4V class star while the secondary is a class M7V.{{cn|date=May 2017}}
The system was observed with the Hubble Space Telescope in the 1990s with its Fine Guidance Sensor.{{Cite journal|last1=Hershey|first1=John L.|last2=Taff|first2=L. G.|date=1998-01-01|title=Hubble Space Telescope Fine Guidance Sensor Astrometry of the Low-Mass Binary L722-22|url=http://stacks.iop.org/1538-3881/116/i=3/a=1440|journal=The Astronomical Journal|language=en|volume=116|issue=3|pages=1440|doi=10.1086/300516|issn=1538-3881|bibcode = 1998AJ....116.1440H |doi-access=free}} This data helped determine the mass of each of the components of L722-22/ LHS 1047 / GJ 1005.
References
{{reflist}}
{{Nearest star systems|4}}
{{Stars of Cetus}}
{{DEFAULTSORT:GJ 1005}}