6. With a combination of large radio telescopes, astronomers can examine the bright star known as Betelgeuse in the constellation of Orion. Betelgeuse is one of the largest stars found in the universe, called a Red Supergiant. We originally thought this star to be 520 light years away (which is equivalent to almost 3,000,000,000,000,000 or 3 x 1015 miles away!) As big as this star really is, in the telescope image, this star appears to be only 0.02 arc-seconds large. Use equation (3) to determine the actual diameter of the star (in miles). Compare that to the size of Earth's orbit around the Sun, about 93 million miles in radius, and comment on the size of Betelgeuse compared to the size of our planet's orbit. Angle of 0.02 arc seconds radio telescope Distance to Betelgeuse=520 light years = 3,000,000,000,000,000 miles Diameter of Betelgeuse:_ Comments on the size of the star: Unit: Betelgeuse c) Determining Diameter from Angular Size and Distance Sometimes astronomers can determine an object's distance using other methods; if you also know the object's angular size in degrees, you can determine its actual diameter using: (3) Small object's diameter Angular Size (in degrees) x Object's distance 57.3 distance and its diameter will be given in the same units.
Stellar evolution
We may see thousands of stars in the dark sky. Our universe consists of billions of stars. Stars may appear tiny to us but they are huge balls of gasses. Sun is a star of average size. Some stars are even a thousand times larger than the sun. The stars do not exist forever they have a certain lifetime. The life span of the sun is about 10 billion years. The star undergoes various changes during its lifetime, this process is called stellar evolution. The structure of the sun-like star is shown below.
Red Shift
It is an astronomical phenomenon. In this phenomenon, increase in wavelength with corresponding decrease in photon energy and frequency of radiation of light. It is the displacement of spectrum of any kind of astronomical object to the longer wavelengths (red) side.
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