Oct 24, 2024 · V0391 Pegasi b is a gas giant exoplanet that orbits a B-type star. Its mass is 3.2 Jupiters, it takes 3.2 years to complete one orbit of its star, and is 1.7 AU from its star. Its …

V391 Pegasi b, also known as HS 2201+2610 b, is an extrasolar planet candidate orbiting the star V391 Pegasi approximately 4,570 light-years away in the constellation of Pegasus. The …

The planet discovered by the researchers, "V 391 Pegasi b," has survived all those changes to its sun. This image represents planet "V 391 Pegasi b" as it survives the red giant expansion of …

Sep 12, 2007 · Researchers believe V391 Pegasi is such a star, called a B subdwarf, that shrunk from about 0.9 solar mass during its youth to 0.5 solar mass today. It is also one of a handful …

V391 Pegasi, also catalogued as HS 2201+2610, is a blue-white subdwarf star approximately 4,400 light-years away in the constellation of Pegasus. The star is classified as an "extreme …

Oct 10, 2024 · V391 Peg b is a Confirmed extrasolar planet (exoplanet) that orbits the star V391 Pegasi in the constellation of Pegasus

Mar 1, 2009 · The pulsating subdwarf B star V 391 Pegasi (or HS 2201+2610), which is close to the two known hybrid pulsators in the log $g$–$T_{\rm eff}$ plane, has recently been …

V391 Pegasi b, also known as HS 2201+2610 b, is an extrasolar planet candidate orbiting the star V391 Pegasi approximately 4,570 light-years away in the constellation of Pegasus. The …

Analysis of 13 years of photometric data for the pulsating sdB star V391 Peg indicated that the pulsation modes agree less well than before, making the presence of a planet orbiting the star …

Jun 29, 2018 · V391 Peg (alias HS 2201+2610) is a subdwarf B (sdB) pulsating star that shows both p - and g -modes. By studying the arrival times of the p -mode maxima and minima …