HR 5110
id:
hr-5110-200-12768141
title:
HR 5110
text:
HR 5110, also known as BH Canum Venaticorum, is a binary star system in the northern constellation of Canes Venatici. It is visible to the naked eye with an apparent visual magnitude of 4.91. Based upon an annual parallax shift of 21.90±0.23 mas, it is located 149 light-years away. The system is moving further from the Sun with a heliocentric radial velocity of 6.4 km/s. This is a close binary system with an orbital period of 2.6 days and an orbital plane that is oriented nearly face-on. It may
brand slug:
wiki
category slug:
encyclopedia
description:
Star in constellation Canes Venatici
original url:
https://en.wikipedia.org/wiki/HR_5110
date created:
date modified:
2023-05-03T14:59:51Z
main entity:
{"identifier":"Q4835609","url":"https://www.wikidata.org/entity/Q4835609"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/8/8e/BHCVnLightCurve.png","width":1500,"height":975}
fields total:
13
integrity:
15