Chapter 1 Flashcards
The average distance from the Earth to the Sun, 149,600,000 km can be written in shorthand notation as-
1.496 x 10 ^8 km
There are 1000 mm in 1 m. This
means that a distance of 10mm is-
1 x 10 ^-2 m
10^2 x 10^5 =
10,000,000
100 (10 ^0) =
1
10^-3 x 10^3 =
1
(3 x 10^4)^4=
8.1 x 10^17
(.5)^3 =
0.125
(8.0 x 10^5) / (2 x 10^3) =
400
The ecliptic can be defined as the-
Path traced out by the Sun in our sky over one year against the background stars.
In which direction dies the Sun appear to move along the ecliptic over the course of a year, relative to the background stars?
East
If we could see background stars in the daytime, the Sun would-
Appear to move eastward against them at a rate of 1• per day
The earth would NOT have seasons if-
It’s axis of rotation were perpendicular to its orbital plane
Why do we see different phases of the moon?
The illuminated half if the moon becomes more or less visible from earth as the moon orbits the earth
The phase if the moon when the sun NAND moon have the same right ascension-
New moon
Approximately when dies a full moon rise?
Sunset