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HD 106248, also known as HR 4649, is a solitary, orange hued star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.34, placing it near the limit for naked eye visibility. Based on parallax measurements from Gaia DR3, the object is estimated to be 358 light years away from the Solar System. It appears to be receding with a heliocentric radial velocity of 34.5 km/s. At its current distance, HD 106248's brightness is diminished by 0.32 due to interstellar dust and Eggen (1993) lists it as a member of the old (thick) disk population.

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rdf:type
rdfs:label
  • HD 106248 (en)
  • HD 106248 (zh)
rdfs:comment
  • HD 106248,又名CP-77 804,SAO 256915、HR 4649,是一颗恒星,视星等为6.35,位于銀經301.01,銀緯-15.84,其B1900.0坐标为赤經12h 8m 18.1s,赤緯-78° -15.84′ 2″。 (zh)
  • HD 106248, also known as HR 4649, is a solitary, orange hued star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.34, placing it near the limit for naked eye visibility. Based on parallax measurements from Gaia DR3, the object is estimated to be 358 light years away from the Solar System. It appears to be receding with a heliocentric radial velocity of 34.5 km/s. At its current distance, HD 106248's brightness is diminished by 0.32 due to interstellar dust and Eggen (1993) lists it as a member of the old (thick) disk population. (en)
foaf:name
  • HD106248 (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Chamaeleon_constellation_map.svg
dcterms:subject
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absmag v
  • +1.10 (en)
age gyr
appmag v
b-v
  • +1.21 (en)
class
  • K2/3 III CNII (en)
constell
epoch
  • J2000.0 (en)
gravity
luminosity
mass
metal fe
  • +0.05 (en)
p error
parallax
prop mo dec
  • −20.594 (en)
prop mo ra
  • −4.318 (en)
radial v
radius
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