Astronomy and Earths Motion Flashcards
Keplers 1st law
The path of a satellite around a primary is an ellipse, with the primary located at a focus point of the ellipse
Keplers 2nd law
Satellites sweep out equal areas in equal times
Keplers 3rd law
Orbital velocity changes, its faster when closer and slower when farther
Aphelion is _______ , perihelion is _______
farther, closet
High eccentricity means
more oval and big change in orbital velocity
Low eccentricity means
more circular and small change in orbital velocity
eccentricity formula
e = d (distance between focus pts)/ L (length of major axis)
gravity
force of attraction between any 2 objects
More mass, ____
stronger gravity
Farther =
weaker gravity
ex. 2x farther -> 4x weaker
Inverse square law
ex. 3x closer -> 3² -> 9
Earth ROTATES…
15 degrees/hour
Earth REVOLUTIONS…
~1 degree/day
Jovian plants are
larger, have longer periods of revolution, and are low density
Terrestrial planets are
smaller, shorter periods of revolution, and are high density