HD 39901 is an orange hued star located in the constellation Columba. It is also called HR 2069, which is the star's Bright Star Catalog designation. Eggen (1989) lists it as a member of the old disk population.
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| - HD 39901 (en)
- HD 39901 (sv)
- HD 39901 (zh)
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| - HD 39901 är en ensam stjärna i den södra delen av stjärnbilden Duvan. Den har en skenbar magnitud av ca 6,56 och kräver åtminstone en handkikare för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 5,1 mas, beräknas den befinna sig på ett avstånd på ca 646 ljusår (ca 198 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -10 km/s. (sv)
- HD 39901,又名CD-42 2205,SAO 217599、HR 2069,是一颗恒星,视星等为6.55,位于銀經249.32,銀緯-28.29,其B1900.0坐标为赤經5h 50m 19.7s,赤緯-42° -28.29′ 29″。 (zh)
- HD 39901 is an orange hued star located in the constellation Columba. It is also called HR 2069, which is the star's Bright Star Catalog designation. Eggen (1989) lists it as a member of the old disk population. (en)
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| - HD 39901 is an orange hued star located in the constellation Columba. It is also called HR 2069, which is the star's Bright Star Catalog designation. Eggen (1989) lists it as a member of the old disk population. Despite the HR designation, the object has an apparent magnitude of 6.54, slightly past the limit for the naked eye visibility. As a result, it is barely visible to the unaided eye in the best conditions. Parallax measurements from the Gaia spacecraft place the object 639 light years away. It is approaching the Solar System with a heliocentric radial velocity of −10.3 km/s. At that distance, HD 39901's brightness is diminished by 0.33 magnitudes due to interstellar dust. It has an absolute magnitude of −0.03. This is an evolved red giant star with a stellar classification of K3 III. It has a comparable mass to the Sun but has expanded to 21.9 times the latter's girth. It radiates 143 times the luminosity of the Sun from its photosphere at an effective temperature of 4,373 K. HD 39901 is slightly enriched in heavy elements with a metallicity 120% that of the Sun's. Like most giants, it spins slowly, having a projected rotational velocity lower than 1.6 km/s. (en)
- HD 39901 är en ensam stjärna i den södra delen av stjärnbilden Duvan. Den har en skenbar magnitud av ca 6,56 och kräver åtminstone en handkikare för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 5,1 mas, beräknas den befinna sig på ett avstånd på ca 646 ljusår (ca 198 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -10 km/s. (sv)
- HD 39901,又名CD-42 2205,SAO 217599、HR 2069,是一颗恒星,视星等为6.55,位于銀經249.32,銀緯-28.29,其B1900.0坐标为赤經5h 50m 19.7s,赤緯-42° -28.29′ 29″。 (zh)
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