31 Vulpeculae
id:
31-vulpeculae-315-7584525
title:
31 Vulpeculae
text:
31 Vulpeculae is a binary star system in the northern constellation of Vulpecula. It is visible to the naked eye as a faint, yellow-hued point of light with an apparent visual magnitude of 4.56. The system is located approximately 228 light years away from the Sun based on parallax, and it is drifting further away with a radial velocity of +2.25 km/s. The variable radial velocity of this system was first suspected by German Astronomer Friedrich Küstner in 1914. The system appears as a single-lin
brand slug:
wiki
category slug:
encyclopedia
description:
Star in the constellation Vulpecula
original url:
https://en.wikipedia.org/wiki/31_Vulpeculae
date created:
date modified:
2023-09-12T14:05:17Z
main entity:
{"identifier":"Q255527","url":"https://www.wikidata.org/entity/Q255527"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/9/94/Vulpecula_constellation_map.svg","width":320,"height":249}
fields total:
13
integrity:
15