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Pathways to Astronomy

Stephen E. Schneider

Chapter 56

The Masses of Orbiting Star - all with Video Answers

Educators


Chapter Questions

03:08

Problem 1

Two stars are in a binary system. Find their combined mass if they have
a. an orbital period, $P$, of 5 years and an orbital separation, $a$, of $10 \mathrm{AU}$.
b. an orbital period, $P$, of 2 years and an orbital separation, $a$, of $4 \mathrm{AU}$.

Andy Chen
Andy Chen
Numerade Educator
02:19

Problem 2

Mizar A and B are about 400 AU apart, currently. Their orbital period is estimated to be between 2000 and 4000 years. What range of masses does this suggest for the pair?

Narayan Hari
Narayan Hari
Numerade Educator
07:44

Problem 3

Two stars are orbiting each other, and the sum of their masses is $6 M_{\odot} .$ It is found that star $A$ of the pair is orbiting 3 arcsec from the center of mass, while star $B$ is orbiting 6 arcsec from the center of mass. What are the two stars' masses?

Eduard Sanchez
Eduard Sanchez
Numerade Educator
04:15

Problem 4

Find the distance from the center of the Sun of the center of mass between the $\operatorname{Sun}\left(M_{\odot}=1.99 \times 10^{30} \mathrm{kg}\right)$ and the following planets:
a. Earth $\left(M=5.97 \times 10^{24} \mathrm{kg} ; a=1.50 \times 10^{8} \mathrm{km}\right)$
b. Jupiter $\left(M=1.90 \times 10^{27} \mathrm{kg} ; a=7.78 \times 10^{8} \mathrm{km}\right)$
c. Saturn $\left(M=5.68 \times 10^{26} \mathrm{kg} ; a=1.43 \times 10^{9} \mathrm{km}\right)$

Ajay Singhal
Ajay Singhal
Numerade Educator
02:37

Problem 5

When Jupiter and Saturn are on the same side of the Sun, is the center of mass inside or outside the Sun's radius $\left(R_{\odot}=6.96 \times\right.$ $\left.10^{5} \mathrm{km}\right) ?$

Arun Bana
Arun Bana
Numerade Educator
06:36

Problem 6

Two stars are orbiting each other, both 4.2 arcsec from their center of mass. Their orbital period is 420.3 years and their distance from the Earth is 104.1 ly. Find their masses.

Matthew Miranda
Matthew Miranda
Numerade Educator
06:36

Problem 7

Using Kepler's third law, we find that the combined mass of a binary system is $55.5 \mathrm{M}_{\odot} .$ The stars have separations of 6.3 arcsec and 2.5 arcsec from the center of mass, and the system is at a distance of 64 ly from the Earth. Find their distances from the center of mass of the system, and their individual masses.

Matthew Miranda
Matthew Miranda
Numerade Educator