Question not worded well. Sounds like right out of homework.
Do I read "low surface" temperature? -- Large diameter relative to the Sun?
By the HR classification, we might be talking about a giant star or a supergiant, or even a hypergiant -- certainly not a main sequence star.
A lower surface temperature, say a K class, or M, or even L, indicates that the star would appear orange to red in color, if it is capable of visible emission.
The largest stars - that is, largest in diameter - are usually red. This is related to the fact that their surface temperature is relatively low. They still radiate huge amounts of energy though, due to their large surface.
The largest stars - that is, largest in diameter - are usually red. This is related to the fact that their surface temperature is relatively low. They still radiate huge amounts of energy though, due to their large surface.
A supergiant simply is a large giant - so, it is larger (in diameter) than a "regular" giant star.
I don't know whether such a star exists, but that might be the case for a star with an extremely large diameter.
It would look brighter if it is closer to Earth. It is also possible for a small star (small in diameter) to have a higher surface temperature, i.e., to emit more light per square meter of its surface.
The absolute magnitude of a start will increase both:* If its surface temperature increases, and * If its diameter increases.
To be bright you need to be hot, close or have a large surface area. The brightest coolest stars are red super giants. They have such a large surface area, that even though their surface temperature is cool - in star terms - their large surface area makes them appear bright.
it is a very large star of high luminosity and low surface temperature.....=)))))
No. I assume you mean the star's diameter. The area is proportional to the square of the area - so the bigger the star, the brighter it will be - other things being equal. However, the star's surface temperature also affects its brightness.
It is a large star
the diameter is 87 meters
A diameter is the distance from one side of a spherical or circular object, through the centre, to the other. It can be as small as an atomic sub-particle or as large as a red super-giant star. There is absolutely no way that 6 millimetres can be "converted" to diameter.