- X -98
- Y -13
- Z 304
- Infra-Red source
- UV-emission source
Gamma Scuti (γ Sct, γ Scuti) is a star in the constellation Scutum.
Gamma Scuti is a white A-type main-sequence star with an apparent magnitude of +4.67. It is approximately 319 light years from Earth.
Currently it is moving towards the Solar System at 41 km/s, which means in 2.1 million years it will pass at just 14 ly distance, probably becoming the brightest star in the night sky, at magnitude -2.1, for a period.This article uses material from the Wikipedia article "Gamma Scuti", which is released under the Creative Commons Attribution-Share-Alike License 3.0.