Access over 35 million academic & study documents

Solar Stellarium

Content type
User Generated
Subject
Physics
School
Florida State University
Type
Homework
Showing Page:
1/6
1
PHYSICS 115 ASTRONOMY-STARS AND GALAXIES
Student Name: …………………………………………… Date: ….....
Student ID: ……………………………………………
Lab 2: Solar & Sidereal Day
Introduction
Some of our most basic knowledge of astronomy is based on observing the sun and
its position in the sky. Unfortunately, some of things we "know" are not entirely
correct! One common misconception is that the sun is directly overhead at noon.
Whether or not the sun is straight overhead depends on where you are on the globe,
what time of year it is, and what you mean by "noon." Similarly, we all know that
one day is 24 hours long. Our entire calendar is based on this fact! However, the
measurement of the rotation rate of any object must be done with respect to some
reference point. When we measure the time it takes for the Earth to complete one
full rotation, it turns out that it makes a difference whether we measure it with
respect to the sun or with respect to a distant star.
Objectives
Clearly define the concept of solar noon
Examine the position of the sun in the sky over the course of a year
Compare the position of the sun at the same time in different global locations
Observe the lengths of solar and sidereal days
Procedure
Launch the Stellarium program and set your location for right here in North
Charleston SC. Make sure you are located at the correct place on the map before
you continue. If it is not already, make this your default location (so that the
program will automatically place you at the correct location on startup).
Noon Is 12:00, Right?
Again, we all know when noon is...it's 12:00 noon. The sun is straight overhead at
noon, right? Check it.

Sign up to view the full document!

lock_open Sign Up
Showing Page:
2/6
2
1. Locate the sun: For the four dates shown below, find the sun at noon exactly
(12:00). Record the Az/Alt coordinates of the sun on each of these days.
A more precise definition for solar noon is the time when the sun crosses the
meridian (the imaginary line from due N to due S can be turned on from the
Viewing Options window). Toggle the meridian on.
2. Is the sun on the meridian? On any of the days you observed, is the sun on the
meridian (az = 180° is the meridian) at noon? No. Is 12:00 on the clock before or
after solar noon for our location? 12:00 on the clock is before the solar noon in
the location.
Date
12:00 Noon
Sun Crosses Meridian
Az
Alt
Time
Az
Alt
09/21/2020
+149°
+53°
13:13
+180°
+57°
12/21/2020
+175°
+34°
12:19
+180°
+34°
03/21/2020
+143°
+52°
13:27
+180°
+58°
06/21/2020
+112°
+70°
13:22
+180°
+81°
3. Find solar noon: Advance the time until the sun crosses the meridian. For each
of the four dates, record the time and the az/alt coordinates.
4. Is the sun directly overhead? On any of the days you checked, does the sun ever
reach an altitude of 90° (directly overhead)?
On any of the days checked, the sun does not ever reach an altitude of 90°.
5. Where will the sun be directly overhead? The figure below shows the positions
of the sun for an observer located at 32°N latitude (Hey! We are located at 32°N
latitude!). Use this figure to help you determine at what northern latitude the sun
will be directly overhead on June 21. Where will the sun be if you are in a
location 10° south of this latitude?
The sun is directly overhead the observer.

Sign up to view the full document!

lock_open Sign Up
Showing Page:
3/6

Sign up to view the full document!

lock_open Sign Up
End of Preview - Want to read all 6 pages?
Access Now
Unformatted Attachment Preview
PHYSICS 115 ASTRONOMY-STARS AND GALAXIES Student Name: …………………………………………… Date: …..... Student ID: …………………………………………… Lab 2: Solar & Sidereal Day Introduction Some of our most basic knowledge of astronomy is based on observing the sun and its position in the sky. Unfortunately, some of things we "know" are not entirely correct! One common misconception is that the sun is directly overhead at noon. Whether or not the sun is straight overhead depends on where you are on the globe, what time of year it is, and what you mean by "noon." Similarly, we all know that one day is 24 hours long. Our entire calendar is based on this fact! However, the measurement of the rotation rate of any object must be done with respect to some reference point. When we measure the time it takes for the Earth to complete one full rotation, it turns out that it makes a difference whether we measure it with respect to the sun or with respect to a distant star. Objectives • • • • Clearly define the concept of solar noon Examine the position of the sun in the sky over the course of a year Compare the position of the sun at the same time in different global locations Observe the lengths of solar and sidereal days Procedure Launch the Stellarium program and set your location for right here in North Charleston SC. Make sure you are located at the correct place on the map before you continue. If it is not already, make this your de ...
Purchase document to see full attachment
User generated content is uploaded by users for the purposes of learning and should be used following Studypool's honor code & terms of service.
Studypool
4.7
Indeed
4.5
Sitejabber
4.4