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Solving the mass and density of celestial bodies

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Solving the mass and density of celestial bodies

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"Gravitation" topic 1 Solving the mass and density of celestial
bodies


Model 1 (orbiting method) assumes that the orbital radius of the satellite

orbiting the object is r, the period is T, the radius of the central object is

R, and the gravitational constant is G.

(1)Try to write an expression for the mass and average density of the central

object? When the satellite moves around the surface of the central object, its

period is T, then the expression for the average density of the central object

is?

(2)If the radius of the orbit around the object is unknown, what physical

quantity needs to be measured and the expression for the mass of the central

object is written?




Model 2 (gravitational acceleration method).Ignoring the rotation of the central

celestial body, it is known that the mass of an apple on the surface of the star

is m, the radius is R, the gravitational acceleration on the surface of the star

is g, and the gravitational constant is g.

(1) Calculate the mass and density of the star

(2) Find the gravitational acceleration g1 of the object at h distance from the

surface of the star

(3) Find the ratio of g to g1

(4) If the rotation of the star is not negligible, the gravitational acceleration

of the two stages of the star and the equator are g pole and g0 respectively,

the rotation period of the star is T, and the mass and density of the star are ?




Single-choice questions
1. Saturn's largest moon is called "Titan" (pictured), which orbits Saturn once




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, every 16 days, and its orbital radius is about 1.2 106 km , and if the

gravitational constant is known G = 6.67 10−11 N  m2 / kg 2 , the mass of Saturn is

about ( ).

A. 5 1017 kg B. 5 1026 kg

C. 7 1033 kg D. 4 1036 kg



2. In April 2021, the core module of China's self-developed space station

"Tianhe" was successfully launched and put into orbit, and the operation of the

core module around the earth can be regarded as a uniform circular motion. The

gravitational constant is known, and the mass of the Earth can be calculated

from the following physical quantities ( )

A. Mass of the core module and radius around the ground

B. Mass of the core module and the period around the ground

C. Angular velocity and circum-earth period of the core module

D. Ground velocity and period around the core module



Multiple-choice questions
3. Two scientists were awarded the 2020 Nobel Prize in Physics for the

discovery of a supermassive compact object at the center of the Milky Way. They

continued to observe the position of a star near the center of the Milky Way

S 2 , and recorded S 2 an elliptical orbit as shown in the figure. O is a focal

point of an ellipse, and the eccentricity (eccentricity) of the ellipse is

about 0.87. P and Q are the far galactic and perigalactic points of the orbit,

respectively, and the distance between Q and O is about120AU (the distance

from the sun to the earth 1AU ), S 2 and the orbital period is about 16 years.

The hypothetical S 2 trajectory is mainly affected by the gravitational pull of

the compact object at the center of the Milky Way, and based on the above data

and daily astronomical knowledge, ( ) can be deduced

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Subido en
7 de julio de 2025
Número de páginas
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Escrito en
2024/2025
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