To determine the lifetime of a 1.43MSun star, we use the formula for stellar lifetimes. Sun 2.5 tsun tstar M. star Using the given mass and multiplying by the expected lifetime of the Sun (11 x 10° years), we can calculate the following. (Round your answer to at least three significant figures.) tstar = years
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.
A 1.43MSun main sequence star is found to have a planet in its habitable zone. What is the expected lifetime (in years) of the star? (Assume that the expected lifetime of the Sun is 11 ✕ 109 years. Round your answer to at least three significant figures.)
![A 1.43Msun main sequence star is found to have a planet in its habitable zone. What is the expected lifetime
(in years) of the star? (Assume that the expected lifetime of the Sun is 11 x 10° years. Round your answer to
at least three significant figures.)
-Age of humans
First anthropoids Age of
mammals
Dec
Life on land
Tertiary
First horses
Cambrian period
Nov
100- Cretaceous
First flowering
plants
Oct
1-
Age of
reptiles
(dinosaurs)
First birds
Jurassic
Sept
200 -
First primitive
mammals
Triassic
Precambrian
Aug
period
Last
Permian
trilobites
2-
Age of
amphibians
July
300ennsylvaniar
Coal-lorming
forests
June
Mississippian
First forests
Devonian
Age of
fishes
May
400
First life on land
3-
Silurian
Аpril
Age of
marine
invertebrates
Ordovician
Origin of life
500 -
March
Carmbrian
-Cambrian
Feb
explosion
Precarmbrian
Ocean life only
600 -
Jan
4.6-
Formation of Earth
Using the figure above, if Earth orbited this star, how far along the timeline would it get?
Part 1 of 2
To determine the lifetime of a 1.43Mun star, we use the formula for stellar lifetimes.
2.5
Msun
tstar
tsun
M
star
Using the given mass and multiplying by the expected lifetime of the Sun (11 x 10° years), we can calculate
the following. (Round your answer to at least three significant figures.)
star
years
Billion yean ago
Million years ago](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F774bf996-e9c6-4d9a-8ddc-e817ff6a1997%2F9b0fe4de-da2f-42f7-9ee1-37c1031e156b%2Fkha9ec_processed.jpeg&w=3840&q=75)
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