Ok, I did a preliminary check on the Extrasolar Planet Encyclopedia; I converted
all stellar apparent magnitudes to absolute magnitudes, those to luminosity (* solar), and calculated the inner and outer boundaries of the HZ, generously assuming an inner edge of 0.9 AU and an outer edge of 1.5 AU for our own solar system.
Not exact matches
«We have carefully examined the early data of the Subaru Strategic Survey with HSC and found an
apparent over density of stars in Virgo with very high statistical significance, showing a characteristic pattern of an ancient
stellar system in the color -
magnitude diagram,» he said.
The system is composed of a blue - white giant with the
stellar classification of B9III - IV and a visual
magnitude of 5.33, a white subgiant belonging to the
stellar class A0IVMn with an
apparent magnitude of 5.63, and a star with a
magnitude of 8.5 separated from the second component by 37.7 arc seconds.