Lab #2 Stellarium AST
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Southcentral Kentucky Community and Technical College *
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195
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Aerospace Engineering
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Feb 20, 2024
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Lab 01: Introduction to Stellarium
Introduction
Stellarium is a free, open-source planetarium program available for download. If you have your own computer, you
should consider installing it. If you have your own copy installed, you can work on lab exercises at your own convenience, review or double-check your lab answers before quizzes, or just play around with it. The program can
be downloaded at: http://www.stellarium.org
. This program is also installed in the physics lab, so you are free to use it any time the lab is open. The advantages of using a computer-generated sky are numerous. First, and most obviously, it’s never too cloudy to observe the sky on the screen! Another powerful advantage is time. We can examine the sky on any day, at any time: past, present, or future. We can watch the stars and planets move quickly across the night sky in a way that would not be possible outdoors, or even with a professional telescope. We can change our location, and see the sky from parts of the world we have never visited...or from other worlds entirely.
Objectives
✦
Become familiar with the Stellarium program and its user interface
✦
Define and distinguish between systems of astronomical coordinates
✦
Examine the position of the sun in the sky over the course of a year
Procedure
Launch the Stellarium program. When the program has loaded, your screen should show you located in a field of grass, facing south. You have two toolbars that you activate by moving the mouse over their locations. At the left edge of the window, towards the bottom, you will find a vertical toolbar with configuration windows for setting location, date, and viewing options. There is a horizontal toolbar along the bottom left edge as well. This has toggles for the most common viewing options, as well as time controls. You can spend a few minutes clicking around, just to see what this button or that toggle does.
Opening Screen
Location Data for Bowling Green, KY
OK, enough fun – time to work
1.
Set your location:
Click on the Location Window icon (vertical toolbar, top icon). There are many ways to specify where you are, but start by doing the fastest thing. In the search box (the part with the magnifying glass), start typing “Bowling Green.” By the time you are three letters in, you should see your location list has been whittled down to just a few places, and you can select Bowling Green, KY. (if there’s no entry for Bowling
Green, you can add it in manually using the location in the image above). Notice on the map that your red location arrow is correctly pointing to central Kentucky, and you can close the location window.
2.
Set your time:
Click on the Date/Time Window icon (vertical toolbar, second icon). It should initially display the current and correct date and time. Let’s go ahead and see the eastern sky earlier this morning. Change the time to 6:00AM, and notice how dramatically your view changes. Go ahead and close the date/time window. 3.
Return to right now:
Activate the horizontal toolbar by moving your mouse over it. The icons on the right end of the toolbar control the passage of time. Click on the “Set time to now” icon, or just type the number 8. You will notice that there are keystrokes which correspond to these toggles, and you will probably find a few that you use frequently—knowing a few keystrokes can be a real timesaver. 4.
Wander around:
Explore your landscape. You can navigate using the mouse or the arrow keys. Spin around, look up, look down. Astronomical Coordinate Systems There are several systems that can be used to locate objects in the sky. We will distinguish here between two coordinate systems: azimuth/altitude (Az/Alt) and right ascension/declination (RA/DE)
. Either one of these systems is analogous to using x- and y-coordinates on a piece of graph paper. They are two dimensional systems, which means that they can tell you where to look in the sky to find an object, but not how far away that object is from the Earth. 5.
Turn and face north:
Toggle on the Azimuthal grid (z), look up a bit, and
examine the coordinate system. Azimuth is the angle measured in a
horizontal circle, around your horizon. Due N = 0°. Head around the circle,
and E = 90°, S = 180°, W = 270° and back to N = 360°. Altitude is the angle
measured from the horizon (0°) to the zenith (90°, or directly overhead).
Thus, any point in the sky that you can see can be specified by telling you
which direction to face (az), and how high up to look (alt). 6.
Set your time for today at 9:00PM (21:00)
: Locate the star Polaris
, and record its az/alt coordinates (click on the star, and notice the information that appears in the top left of your screen). Pay attention to how these coordinates correspond to the star’s location in the sky. 359°34'12.5" +37°32'16.6"
7.
Toggle between mounts:
Notice the difference between the equatorial and
azimuthal mounts! The azimuthal mount parallels the az/alt coordinates.
The equatorial mount makes no sense if you imagine you are outside
looking at the sky with your naked eye, but makes sense if you imagine that
you are looking through the eyepiece of a telescope. Many telescopes are
mounted parallel to the celestial equator, which makes adjusting to find
objects easy using RA/DE coordinates. (1pt) Does changing the telescope
mount change the actual location of the object?
No, changing the telescope does not alter the location of the object.
8.
Toggle between grids:
Turn off the az/alt coordinates (z), and toggle on the equatorial grid (e). You are now looking at the right ascension/declination coordinate system. Record these coordinates for Polaris
, and notice that RA is not given in degrees. Always use the J2000 coordinates for RA/DE.
03h 02m56.9s +89°22'14.2"
9.
Set the day and time:
Change the date to 09/01/14, at 9:00PM (21:00). Locate the bright star Acturus in the western sky. Record both its Az/Alt coordinates and RA/DE
. Move forward in time to 12/01/14 at the same time, and record the positions. Note that even if the star dips below your viewing horizon (alt < 0°), its position
is still displayed. Continue to advance in three month increments for an entire year. (4pt) Arcturus Coordinates – Bowling Green, KY
Date
Azimuth and Altitude
Right Ascension and Declination
Az
Alt
RA
DE
09/01/14
274°40'31.2"
+26°35'58.1"
14h 16m19.3s
+19°06'38.2"
12/01/14
354°43'54.8"
-33°43'44.5"
14h 16m19.4s
+19°06'21.3"
03/01/15
071°11'14.9"
+06°56'57.7"
14h 16m22.1s
+19°06'05.1"
06/01/15
129°39'49.7"
+64°47'31.0"
14h 16m22.9s
+19°06'16.3"
10.
Change your location:
Return to the original date (09/01/14) and time (21:00). Remain centered on the star Arcturus, but change your observation location. Pick any place you like: New York, Chicago, Paris...literally anywhere. Note your location, and record one more time the Az/Alt and RA/DE coordinates for the star. (4pt) Arcturus Coordinates for City: ______Tokyo, Japan________________________
Date
Azimuth and Altitude
Right Ascension and Declination
Az
Alt
RA
DE
09/01/14
088°50'05.3"
+32°30'26.0"
14h 16m19.3s +19°06'38.1"
12/01/14
256°50'50.5"
+49°55'18.8"
14h 16m19.4s +19°06'21.3"
03/01/15
310°47'00.3"
-17°46'11.7"
14h 16m22.0s
+19°06'05.3"
06/01/15
354°37'25.6"
-35°02'14.0"
14h 16m22.9s
+19°06'11.1"
(1pt) For the location you chose, is Arcturus visible above the horizon?
Only on 09/01 and 12/01.
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