Canes Venatici I
id:
canes-venatici-i-256-8683649
title:
Canes Venatici I
text:
Canes Venatici I or CVn I is a dwarf spheroidal galaxy situated in the Canes Venatici constellation and discovered in 2006 in the data obtained by Sloan Digital Sky Survey. It is one of the most distant known satellites of the Milky Way as of 2011 together with Leo I and Leo II. The galaxy is located at a distance of about 220 kpc from the Sun and is moving away from the Sun at a velocity of about 31 km/s. It is classified as a dwarf spheroidal galaxy (dSph) meaning that it has an elliptical sha
brand slug:
wiki
category slug:
encyclopedia
description:
Galaxy in constellation Canes Venatici
original url:
https://en.wikipedia.org/wiki/Canes_Venatici_I
date created:
date modified:
2024-04-24T00:12:02Z
main entity:
{"identifier":"Q46034","url":"https://www.wikidata.org/entity/Q46034"}
image:
fields total:
13
integrity:
14