Calculate the weight of a 75.6 kg astronaut on the surface of Mars at the equator.See p. 273 of your textbook for Mars' mass and equatorial radius.75 ClumU their ownOnly one Moon (natural satellite)but Jupiter and Saturn have many, and more are being found all thetime. Table 5.6 shows the planets and some of their known moons.V Table 5.5 Solar Celestial BodiesCelestialBodySunMercuryVenusEarthMarsCeresJupiterSaturnUranusNeptunePlutoErisSednaMass(kg)1.99 X 10303.30 × 10234.87 X10245.97 X 10²46.42 × 10239.5 × 10201.90 × 10275.69 × 10268.68 ×102510²61.02 X1.20 × 10²2?4.21 X 10²1EquatorialRadius(m)6.96 X 1082.44 X 1066.05 X 1066.38 X 1063.40 X 1064.88 × 1057.15 X 1076.03 × 1072.56 × 1072.48 X 1071.70 X 106~1.43 X 1068.5 X 105www.NOrbitalPeriod(days)87.97224.7365.24686.931679.84330.610 755.730 687.260 19090 553204 5403 835 020MMean OrbitalRadius(m)5.79 × 10101.08 × 10¹11.49 × 10112.28 ×10114.14 × 10117.78 × 10¹11.43 × 10122.87 × 10124.50 × 10¹25.91 X 1012~1.01 X 10137.14 X 1013Distance(AU)0.3870.72311.5242.7665.2039.53719.19130.06939.48267.940479.5Chapter 5 Newton's laws

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Calculate the weight of a 75.6 kg astronaut on the surface of Mars at the equator See p. 273 of your textbook for Mars' mass and equatorial radius.

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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Concept explainers

Centripetal Force

A particle, body, object or certain mass while travelling in a rotational path or semicircular path, experiences an inertia force. If that inertia force pulls the towards the inward of the imaginary circle in the rotation, it is termed as centripetal force.

Question

Calculate the weight of a 75.6 kg astronaut on the surface of Mars at the equator.
See p. 273 of your textbook for Mars' mass and equatorial radius.
75 Clu
m
U

their own
Only one Moon (natural satellite)
but Jupiter and Saturn have many, and more are being found all the
time. Table 5.6 shows the planets and some of their known moons.
V Table 5.5 Solar Celestial Bodies
Celestial
Body
Sun
Mercury
Venus
Earth
Mars
Ceres
Jupiter
Saturn
Uranus
Neptune
Pluto
Eris
Sedna
Mass
(kg)
1.99 X 1030
3.30 × 1023
4.87 X
1024
5.97 X 10²4
6.42 × 1023
9.5 × 1020
1.90 × 1027
5.69 × 1026
8.68 ×
1025
10²6
1.02 X
1.20 × 10²2
?
4.21 X 10²1
Equatorial
Radius
(m)
6.96 X 108
2.44 X 106
6.05 X 106
6.38 X 106
3.40 X 106
4.88 × 105
7.15 X 107
6.03 × 107
2.56 × 107
2.48 X 107
1.70 X 106
~1.43 X 106
8.5 X 105
www.N
Orbital
Period
(days)
87.97
224.7
365.24
686.93
1679.8
4330.6
10 755.7
30 687.2
60 190
90 553
204 540
3 835 020
M
Mean Orbital
Radius
(m)
5.79 × 1010
1.08 × 10¹1
1.49 × 1011
2.28 ×
1011
4.14 × 1011
7.78 × 10¹1
1.43 × 1012
2.87 × 1012
4.50 × 10¹2
5.91 X 1012
~1.01 X 1013
7.14 X 1013
Distance
(AU)
0.387
0.723
1
1.524
2.766
5.203
9.537
19.191
30.069
39.482
67.940
479.5
Chapter 5 Newton's laws

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