Galactic orientation
id:
galactic-orientation-197-3984027
title:
Galactic orientation
text:
Galactic clusters are gravitationally bound large-scale structures of multiple galaxies. The evolution of these aggregates is determined by time and manner of formation and the process of how their structures and constituents have been changing with time. Gamow (1952) and Weizscker (1951) showed that the observed rotations of galaxies are important for cosmology. They postulated that the rotation of galaxies might be a clue of physical conditions under which these systems formed. Thus, understan
brand slug:
wiki
category slug:
encyclopedia
description:
original url:
https://en.wikipedia.org/wiki/Galactic_orientation
date created:
date modified:
2022-01-18T20:15:08Z
main entity:
{"identifier":"Q3356302","url":"https://www.wikidata.org/entity/Q3356302"}
image:
fields total:
13
integrity:
13