WASP-26 is a G-type subgiant star about 824 light-years away in the constellation of Cetus.
WASP-26 is a G-type subgiant star about 824 light-years away in the constellation of Cetus.
== Star characteristics == WASP-26 is an old star close to leaving the main sequence and is part of a wide binary. The binary's projected separation is 3800 astronomical units, its companion star being a K-type star with an effective temperature of 4600K and a visual magnitude of 13.6. WASP-26 produces a large amount of ultraviolet light due to frequent flares, with an average ultraviolet flux close to the F7 class main-sequence star WASP-1.
Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).