I need the answer to part D please! i posted the text from book with answer, but
ID: 114789 • Letter: I
Question
I need the answer to part D please! i posted the text from book with answer, but cant seem to get it correct. ANSWER SHOULD BE A NUMBER AND TWO WORDS.
In 1690, Cassini noticed that the speeds of Jupiter’s clouds vary with latitude, an effect called differential rotation. Near the poles, the rotation period of Jupiter’s atmosphere, 9 h 55 min 30 s, is 5 min longer than at the equator. Furthermore, clouds at different latitudes circulate in opposite directions—some eastward, some westward. At their boundaries, the clouds rub against each other, cre- ating beautiful swirling patterns (see Figures 7-2, 7-4, and 7-5c). The interactions of clouds at different latitudes also help provide stability for storms like the Great Red Spot.
Explanation / Answer
D) Near the poles, the rotation period Of Jupiter's atmosphere is "5 minutes longer " than at the equator. (one number and two words)