RS Sagittarii
id:
rs-sagittarii-292-9696884
title:
RS Sagittarii
text:
RS Sagittarii is an eclipsing binary star system in the southern constellation of Sagittarius, abbreviated RS Sgr. It is a double-lined spectroscopic binary with an orbital period of 2.416 days, indicating that the components are too close to each other to be individually resolved. The system has a combined apparent visual magnitude of 6.01, which is bright enough to be faintly visible to the naked eye. During the primary eclipse the brightness drops to magnitude 6.97, while the secondary eclips
brand slug:
wiki
category slug:
encyclopedia
description:
Eclipsing binary star system in the constellation Sagittarius
original url:
https://en.wikipedia.org/wiki/RS_Sagittarii
date created:
date modified:
2023-12-03T01:37:03Z
main entity:
{"identifier":"Q6095831","url":"https://www.wikidata.org/entity/Q6095831"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/4/42/RSSgrLightCurve.png","width":1500,"height":975}
fields total:
13
integrity:
15