Calculate the Hubble constant Ho. (Round your answer in km/s/Mpc to at least the nearest integer.) H₂ = km/s/Mpc Estimate the Hubble time (in yr). years Is your result similar to the value of Ho = 70 km/s/Mpc? (Choose 'Yes' if your result for Ho agrees to within 5% of the accepted value of 70 km/s/Mpc. Otherwise, choose 'No'.) Ⓒ Yes O No
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.
Use the data in the figure below to complete the following exercises.
Plot a velocity-distance diagram. Plot velocity on the vertical axis and distance on the horizontal axis. Circle the data points on the diagram that you will use to determine H0.
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