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fixed spelling errors
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@ -9,7 +9,7 @@ of this file.
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The derivation shows that a projectile does not need to aim directly at the target
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body in order to hit it, as R_capture>R_target. Astronomers refer to the effective
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cross section for caputre as σ=π*R_capture**2.
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cross section for capture as σ=π*R_capture**2.
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This algorithm does not account for an N-body problem.
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@ -22,7 +22,7 @@ def capture_radii(
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projectile_velocity: float
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)->float:
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#Gravitational constant to four signifigant figures as of 7/8/2023|
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#Gravitational constant to four significant figures as of 7/8/2023|
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#Source google: gravitational constant
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g=6.6743e-11 #SI units (N*m**2)/kg**2
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@ -117,5 +117,5 @@ Let: Mt=target mass, Rt=target radius, v=projectile_velocity,
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Source: Problem Set 3 #8 c.Fall_2017|Honors Astronomy|Professor Rachel Bezanson
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Source #2: http://www.nssc.ac.cn/wxzygx/weixin/201607/P020160718380095698873.pdf
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8.8 Planetary Rendevous: Pg.368
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8.8 Planetary Rendezvous: Pg.368
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"""
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