Title: There is a time''TURN TURN TURN
1There is a time..TURN TURN TURN
2What is a Day?
We start with the Sun, Earth, and person in the
beginning orientation, Noon.
The Sun is directly overhead of the person in a
particular position on the Earth. The Earth is
also spinning about its axis as the day
progresses carrying the person along with it.
Earths Revolution
Earths Rotation
3Sidereal Day
One Sidereal Day23h 56m 4.09s
The earth has made one complete spin on its axis
and returned the person to the original starting
location with respect to the Earth. However,
notice that it is not Noon the next day.
The Sun is not directly overhead of the person
yet. To reach Noon the next day requires the
Earth to spin an additional amount to reach the
same time orientation.
Earths Revolution
One Sidereal Day
Earths Rotation
4Solar Day
One Solar Day24h
Because the Earth moves along its orbit around
the Sun, the Earth must rotate nearly 361o to get
from one local noon to the next.
This extra 1o of rotation corresponds to 4
minutes of time.
Earths Revolution
Earths Rotation
5The CelestialSphere
- Our Earthly Map on the Sky
6Earthly Coordinates
North Pole
N
W
E
S
Our Astronomer is in the northern hemisphere
(like us) and wants to devise a quick way to find
objects and events on the sky.
South Pole
7Move the Coordinates Out!
North Circumpole
Celestial Equator
The Night Sky Celestial Sphere
Eq.
Take the coordinates we have an understanding
about and project them onto the night sky.
South Circumpole
8Add Important Events
N.C.P.
- Now we begin to look for objects, important
events, and observations to add to the celestial
sphere. - Where is the Sun?
- What date is it?
- How are objects moving?
C.E.
S.C.P.
9What happens during the year?
10The Celestial Sphere is Complete!
11Suns Path Winter Solstice
12Suns Path Vernal Equinox
13Suns Path Summer Solstice
14(No Transcript)