Gliese 638 - Wikipedia
Gliese 638 is a main sequence star in the constellation of Hercules. It is located about 32.1 light-years from the Earth. This is a suspected variable star with a measured apparent magnitude …
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Gliese 638 | Stellar Catalog
Nearby star Gliese 638 is a main sequence star that fuses hydrogen atoms into helium. Temperature on its surface is around 4181 K (3908 °C), which is about 72 % of Sun's …
Gliese 638 - Wikiwand
Gliese 638 is a main sequence star in the constellation of Hercules. It is located about 31.9 light years from the Earth. This is a suspected variable star with a measured apparent magnitude …
Gliese 638.1 - star system bodies | Elite:Dangerous | INARA
︎ Gliese 638.1 A 4 - High metal content world Landable. Body distance. 193 Ls. Earth masses. 1.6924. Radius. 7,104 km. Gravity. 1.36 g. Surface temperature. 542 K (269°C/516°F) Surface …
Gliese 638 - Alchetron, The Free Social Encyclopedia
Jan 31, 2024 · Gliese 638 is a main sequence star in the constellation of Hercules. It is located about 31.9 light years from the Earth. This is a suspected variable star with a measured …
Gliese 638 - CaLiGraph
CaLiGraph is a large-scale semantic knowledge graph with a rich ontology which is compiled from the DBpedia ontology, and Wikipedia categories & list pages. View all the information about …
Gliese 638 | Stellar Catalog
Étoile orange Gliese 638 est situé 32 à des années-lumière du soleil. Ce est un seul étoile de classe spectrale K7.5 Ve, qui a généralement environ 70 % de masse solaire. Pour l´instant, il …
Gliese 638 - Wikipedia
Gliese 638 (GJ 638 / HD 151288 / HIP 82003) ye una estrella na constelación d' Hércules asitiada a unos 2º de la brillosa ζ Herculis. De magnitú aparente +8,11, [9] nun ye visible a simple …
Gliese 638.1 - star system | Elite:Dangerous | INARA
The companion site for Elite:Dangerous with the game database, market data, trade routes, outfitting, engineers, blueprints, crafting, Thargoid war, squadrons ...
Gliese 638 - Stellar Catalog
Estrella naranja Gliese 638 se encuentra 32 años luz de distancia del sol. Es un solo estrella de clase espectral K7.5 Ve, que tiene típicamente sobre 70 % de masa solar. Por ahora, no hay …
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