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Homework answers / question archive / Determine the missing values for each different body (1 Newton=0
Determine the missing values for each different body (1 Newton=0.22 lb, 1 lb =4.54 N). Values should be carried out to 2 decimal places when it is not a whole number.
http://hyperphysics.phy-astr.qsu.du/hbase/vesc.html#ves
Use the following applet to calculate the escape velocity. Do not use commas when putting numbers into this applet.
Please see the attached file. This solution consists of all the detailed explanation given at the end, after the table.
http://hyperphysics.phy-astr.qsu.du/hbase/vesc.html#ves
Use the following applet to calculate the escape velocity. Do not use commas when putting numbers into this applet.
1 2 3 4 5 6 7 8
m2 r g a=gx10m/sec2 m1 f=m1x a 0.22f Applet
escape
planet mass planet gravitational acceleration your your your velocity
pull of g mass weight weight km/sec
(earth=1) radius (earth= 1 g) newton pd
(x) (y) g(x/y2)
1 1 1g 10 m/sec2 60kg 600 N 132 11.2
1 2 1(g/4) 2.5 m/sec2 60kg 150 N 33 7.84
2 2 1(g/2) 5.0 m/sec2 60kg 300 N 66 11.2
318 11.2 2.535 g 25.35 m/sec2 60kg 1521N 334.62 59.68
(jupiter)
0.002 0.17 0.069g 0.69 m/sec2 60kg 41.4 N 9.108 1.215
(pluto)
95 9.4 1.075g 10.75 m/sec2 60kg 645 N 141.9 35.6
(saturn)
100,000 0.01 109 g 1010 m/sec2 60kg 6 x 1011 1.32x1011 35420
(neutron
star)
Formulae used in above table:
• Column 3 (g): Gravitational pull:
Gravitatoinal acceleration due to the planet in multiples of g:
Gravitatoinal acceleration due to the planet
For earth, Gravitational acceleration
For a planet with mass m2 =mp = xme and Rp = yRe,
The 1st column of mass m2 denotes the ratio of mass of the planet to that of the earth i.e. (mp/me) while the second column of radius r denotes the ratio of radius of the planet to the radius of the earth.
• Column 4 (a) Gravitational acceleration of the planet:
Gravitational acceleration of the planet: (Column3)x (g due to earth, 10m/s2)
• Column 5 Given
• Column 6 f = ma i.e. f = (column 5) x (column 4)
• Column 7 = 0.22 x (Column 6)
• Column 8 Escape velocity from the surface of a planet
----- (1)
Radius of the planet = y (Radius of the Earth)
i.e. Rp = y Re ----- (a) (Get y from column 2)
From column 3, get gp = (x/y2)g ----- (b)
Substituting (a) and (b) in equation (1), we get
i.e. ---- (2)
Escape velocity from the surface of the earth ---- (3)
[This value is a standard value. If required, it can be calculated by substituting
g = 10 m/s2 and radius of the earth R = 6400 km = 6.4 x 106 m in equation (3) ]
Dividing equation (2) by (3), we get the escape velocity from the surface of the
planet in terms of escape velocity from the surface of the Earth as
i.e. ----- (4)
i.e. in km/s ----- (5)
Use equation (5) for the calculation of the escape velocities for all the planets in last column.
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