HAT-P-15
id:
hat-p-15-246-3827669
title:
HAT-P-15
text:
HAT-P-15 is a G-type main-sequence star about 630 light-years away. The star is older than Sun yet has a concentration of heavy elements roughly 190% of solar abundance. The star has no noticeable starspot activity. The spectroscopic survey in 2015 have failed to find any stellar companions to it, yet imaging survey have identified a possibly two companion red dwarf stars at projected separations 1210 and 1370 AU, respectively. The star was named Berehynia in December 2019 by Ukrainian amateur a
brand slug:
wiki
category slug:
encyclopedia
description:
Star in the constellation Perseus
original url:
https://en.wikipedia.org/wiki/HAT-P-15
date created:
date modified:
2024-04-24T22:27:53Z
main entity:
{"identifier":"Q4039798","url":"https://www.wikidata.org/entity/Q4039798"}
image:
fields total:
13
integrity:
14