 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
q |
Today’s eccentricity is 0.0167, lies well toward the
|
|
|
lower end of the variation range of Earth’s
|
|
|
|
eccentricity (closer to circular).
|
|
|
q |
The long-term variations in orbital eccentricity are
|
|
|
concentrated at two periods: 100,000 years and
|
|
|
|
413,000 years.
|
|
|
q |
The eccentricity variations differ from the other
|
|
|
two orbital variations (obliquity variations and the
|
|
|
|
precessional variations) in one important aspect:
|
|
|
Eccentricity variations cause changes in the
|
|
|
annually averaged amount of sunlight hitting Earth.
|