WR 102ea
id:
wr-102ea-300-252258
title:
WR 102ea
text:
WR 102ea is a Wolf–Rayet star in the Sagittarius constellation. It is the third most luminous star in the Quintuplet cluster after WR 102hb. With a luminosity of 2,500,000 times solar, it is also one of the most luminous stars known. Despite the high luminosity it can only be observed at infra-red wavelengths due to the dimming effect of intervening dust on visual light. It is an evolved massive star which has an emission line spectrum from a strong stellar wind caused by high luminosity and the
brand slug:
wiki
category slug:
encyclopedia
description:
Star in the constellation Sagittarius
original url:
https://en.wikipedia.org/wiki/WR_102ea
date created:
date modified:
2023-03-16T05:56:50Z
main entity:
{"identifier":"Q1090392","url":"https://www.wikidata.org/entity/Q1090392"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/f/fc/Quintuplet_cluster.jpg","width":792,"height":800}
fields total:
13
integrity:
15