Habitability of K-type main-sequence star systems
id:
habitability-of-k-type-main-sequence-star-systems-321-4532846
title:
Habitability of K-type main-sequence star systems
text:
K-type main-sequence stars, also known as orange dwarfs, may be candidates for supporting extraterrestrial life. These stars are known as "Goldilocks stars" as they emit enough radiation in the non-UV ray spectrum to provide a temperature that allows liquid water to exist on the surface of a planet; they also remain stable in the main sequence longer than the Sun by burning their hydrogen slower, allowing more time for life to form on a planet around a K-type main-sequence star. The planet's hab
brand slug:
wiki
category slug:
encyclopedia
description:
Overview of the habitability of K-type main-sequence star systems
original url:
https://en.wikipedia.org/wiki/Habitability_of_K-type_main-sequence_star_systems
date created:
date modified:
2024-03-17T07:55:38Z
main entity:
{"identifier":"Q5636874","url":"https://www.wikidata.org/entity/Q5636874"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/e/eb/MarsCuriosityRover-Drilling-Sol170%2B%2B-2.jpg","width":3819,"height":4223}
fields total:
13
integrity:
15