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==Distance== ==Distance==
In 1991, Gliese ''et al'' gave ] (πp) as 121.8 ± 3.0 ].<ref name="Gliese1991">{{cite book|last1=Gliese|first1=W.|last2=Jahreiß|first2=H.|title=Preliminary Version of the Third Catalogue of Nearby Stars|date=1991|chapter=GI 338|url=http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=V/70A&Name=Gl%20338}}</ref> In 1995, van Altena gave parallax as 122.1 ± 2.9 mas.<ref name="van Altena1995"></ref> In 2014, Dittman ''et al'' gave parallax as 130.60 ± 3.60 mas.{{r|Dittmann2014}}
{{πt}}
{{πp|gj|121.8|3.0|<ref name="Gliese1991">{{plxref|gj=1151}}</ref>}}
{{πp|plx|122.1|2.9|<ref name="van Altena1995">{{plxref|plx=2739.01}}</ref>|b=}}
{{πp|Dittmann ''et al.'' (2014)|130.60|3.60|{{r|Dittmann2014}}}}
{{πe}}


==References== ==References==

Revision as of 08:59, 23 June 2018

GJ 1151 is a red dwarf star of spectral type M4.5V, located in constellation Ursa Major at 26.7 light-years from Earth.

Distance

In 1991, Gliese et al gave parallax (πp) as 121.8 ± 3.0 mas. In 1995, van Altena gave parallax as 122.1 ± 2.9 mas. In 2014, Dittman et al gave parallax as 130.60 ± 3.60 mas.

References

  1. ^ VizieR, Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
  2. Gliese, W.; Jahreiß, H. (1991). "GI 338". Preliminary Version of the Third Catalogue of Nearby Stars.
  3. Attention: This template ({{cite doi}}) is deprecated. To cite the publication identified by doi:10.1088/0004-637X/784/2/156, please use {{cite journal}} (if it was published in a bona fide academic journal, otherwise {{cite report}} with |doi=10.1088/0004-637X/784/2/156 instead.
Known celestial objects within 20 light-years
Primary member type
Celestial objects by systems. Secondary members are listed in small print.
    0–10 ly
Main-sequence
stars
A-type
G-type
M-type
(red dwarfs)
Brown dwarfs
L-type
  • Luhman 16 (6.5029±0.0011 ly)
  • T-type brown dwarf B
Sub-brown dwarfs
and rogue planets
Y-type
10–15 ly
Subgiant stars
F-type
Main-sequence
stars
G-type
  • Tau Ceti (11.9118±0.0074 ly)
  • 4 (8?) planets: (b), (c), (d), e, f, g, h, (i)
K-type
M-type
(red dwarfs)
Degenerate
stars
White dwarfs
Brown dwarfs
T-type
15–20 ly    
Subgiant stars
G-type
Main-sequence
stars
A-type
G-type
K-type
M-type
(red dwarfs)
Degenerate
stars
White dwarfs
Brown dwarfs
L-type
T-type
Y-type
Sub-brown dwarfs
and rogue planets
Y-type
Italic are systems without known trigonometric parallax.
Constellation of Ursa Major
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Nebulae
Galaxies
Messier
NGC
Other
Astronomical events
Category

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