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How Powerful Would A Telescope Need To Be To See Vy Canis Majoris? (Solved)

With a typical visual brightness ranging between 7.4 and 9.6, it is bright enough to be viewed through small telescopes or even big binoculars when it is at its brightest. However, because it is red, it is difficult to determine its magnitude, making it a tricky star to observe.
What kind of star is VY Canis Majoris, and what does he look like?

  • The star is classified as a pulsing Slow Irregular variable type, which implies that its size fluctuates over the course of time. In most cases, the Variable Type is named after the very first star of that type to be discovered. The brightness of VY Canis Majoris varies from a magnitude of 8.762 to a magnitude of 7.444 throughout the course of its variable period.

Can you see VY Canis Majoris?

The star is of the Slow Irregular variable type, which indicates that its size fluctuates over time as it pulses. It is customary to name the Variable Type after the first star of that type to be discovered. Over the course of its varied cycle, the brightness of VY Canis Majoris varies from a magnitude of 8.762 to a magnitude of 7.444;

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How long would it take to get to VY Canis Majoris from Earth?

If the star VY Canis Majoris were to pass through the solar system, the Earth would be completely enveloped by the star’s photosphere. If a car traveling at 120 miles per hour were to be on its way to VY Canis Majoris, it would arrive at the star in about years.

What would happen if VY Canis Majoris was our sun?

If our sun were replaced by VY Canis Majoris, the outer layers of the planet would reach beyond the orbit of the fifth planet, Jupiter, according to calculations. Given its distance from us (about 3,900 light-years), it appears to us (with telescopes) as a dim star, despite the fact that it is really 300,000 times brighter than the sun!

Is there anything bigger than VY Canis Majoris?

VY Canis Majoris has been scaled back to its proper proportions. Current thought is that there are seven known stars that are bigger than VY Canis Majoris, the largest of which is UY Scuti, and that there are more unknown stars. According to current theories, the initial generation of stars was much, much bigger than anything we can see now.

How many miles away is VY Canis Majoris?

Complete response: We must be aware that the diameter of VY Canis Majoris is 155000 times greater than the diameter of our planet. Assume that nnumbers of Earths can be squeezed into VY Canis Majoris with no problem. As a result, we may deduce that 7.54771010Earths can be accommodated within VY Canis Majoris’s orbit.

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How long would it take to fly around Betelgeuse?

320,000 years have passed. What if you were to drive around it at a normal speed? What would happen? Only 9,500 years have passed. But no one would do that if they had the option of taking an aircraft.

What is the absolute magnitude of VY Canis Majoris?

Chanel’s first discovery Of course, the most effective method to feel very, extremely, extremely little is to compare our sun to VY Canis Majoris, one of the biggest stars ever discovered. The diameter of this star is approximately 2000 times greater than the diameter of our sun and 155,000 times more than the diameter of the Earth.

What’s the biggest star known to man?

With a radius almost 1,700 times greater than that of the sun, UY Scuti is the biggest star known to have ever existed in our cosmos. And it is not the only star that dwarfs the Earth’s main star.

What is the largest sun ever discovered?

According to the measurements, UY Scuti is the largest and most luminous of the three stars studied, with a radius of 1,708 192 R (1.188109 134,000,000 km; 7.94 0.89 AU) based on an angular diameter of 5.480.10 mas and an assumed distance of 2.90.317 kiloparsecs (kpc) (approximately 9,5001,030 light-years) that was originally derived in 1970.

What is the largest star ever discovered?

However, of all the stars we can see, the biggest is the oddly called UY Scuti, which is around 1,708 192 solar radii and is the largest we can see.

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