62 G. Sco, CD−38° 10983, CPD−38° 6407, FK5 3295, GC 22030, Gl 620.1, HIP 80337, HR 6094, SAO 207622, Wo 9559.[11]
Database references
SIMBAD
data
ARICNS
data
HD 147513 (62 G. Scorpii) is a star in the southern constellation of Scorpius. It was first catalogued by Italian astronomer Piazzi in his star catalogue as "XVI 55".[12] With an apparent magnitude of 5.38,[2] according to the Bortle scale it is visible to the naked eye from suburban skies. Based upon stellar parallax measurements by the Hipparcos spacecraft, HD 147513 lies some 42 light years from the Sun.[1]
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HD147513 (62 G. Scorpii) is a star in the southern constellation of Scorpius. It was first catalogued by Italian astronomer Piazzi in his star catalogue...
HD147513 b is an exoplanet approximately 42 light-years away in the constellation of Scorpius. It is at least 21% more massive than Jupiter. But unlike...
planetary systems with white dwarfs as distant companions (Gl 86, HD 27442, and HD147513), no debris disks had previously been discovered with a closely...
Trojan planets in the habitable zone: an application to the systems HD147513 and HD 210277". Monthly Notices of the Royal Astronomical Society. 423 (4):...
most massive exoplanet candidate is HD 217786 b, which masses 12.98 MJ; the least massive confirmed planet is HD 10180 b, which masses 0.004 MJ or 3.1...