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What else can I help you with?
Is a betelgeuse star a super giant star?
Yes, Betelgeuse is a supergiant star. It is a red supergiant star located in the constellation of Orion and is one of the largest stars known in our galaxy.
Which of these stars is a red supergiant?
A non red giant is a giant, whereas a supergiant is well a supergiant and is a lot bigger.
Is Betelgeuse a dwarf planet?
No, Betelgeuse is not a dwarf planet. Betelgeuse is a supergiant star located in the constellation of Orion. It is one of the largest and most luminous stars known in our galaxy.
Is a galaxy bigger than a neutron star?
No galaxies is way biger than a star, a star is .0000765% of a galaxy.
Is a galaxy bigger then a star?
Yes. A galaxy contains many stars.
Why is a galaxy more likely to collide with another galaxy that a star with another star?
Because there way bigger than the star
Is the star Antares a supergiant?
Yes, it is a red supergiant star.
Which is largest supergiant constellation solar system or galaxy?
A galaxy is larger than a supergiant constellation. A galaxy can contain billions to trillions of stars, while a supergiant constellation refers to a group of stars that form a recognizable pattern in the sky, typically within our own galaxy.
What is the closest galaxy to Rigel star?
The closest galaxy to the star Rigel is the Andromeda Galaxy (M31). Located approximately 2.537 million light-years away from Earth, Andromeda is the nearest spiral galaxy to our Milky Way. Rigel, a blue supergiant star in the constellation Orion, is part of our Milky Way galaxy, making Andromeda the closest significant galaxy in the broader cosmic neighborhood.
What is bigger a star or a galaxy?
Galaxies are made out of many millions of stars.
What is bigger the sun or the Andromeda galaxy?
Lmao, 220,000ly gaalxy vs. a dwarf star that has a diameter of 1.3mln km lmao it's obvious Andromeda is a bigger
How can you find a supergiant star?
The easiest supergiant star to see is Betelgeuse, the bright red star at the shoulder of Orion the Hunter.
