Lab 1- Introduction to Stellarium _
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CHARLESTON SOUTHERN UNIVERSITY
PHYSICS 115 ASTRONOMY-STARS AND GALAXIES
Student Name: Jewel Ash
Date: 10/22/2023
Student ID: 204386
LAB 1: INTRODUCTION TO STELLARIUM
Objectives
Become familiar with the Stellarium program and its user interface
Define and distinguish between systems of astronomical coordinates
Introduction:
In this activity, you will become familiar with the basic workings of the Stellarium program and
you will be introduced to many of the procedures you will be asked to follow for other lab
assignments in the course. Be sure to answer all of the questions.
Installing the program:
To run the program at home, you will need to install the program to
your hard drive. Please access the website https://stellarium.org/ to obtain the free software.
Stellarium also has a user guide available.
Install the appropriate version for your operating system. When you click the version to install, the
download should begin automatically after the next page loads.
Windows users:
Newer computers
have 64-bit processors, but you can check using instructions found online.
http://windows.microsoft.com/en-us/windows/32-bit-and-64-bit-windows#1TC=windows-7
.
To take the software out of full-screen mode, click the button shown to the right or click F11.
(You
may
have
to
hold
Fn.)
1
Fig 1.
Start up the program. Once the main window pops up, you should be acquainted with the layout
of the main interface. At the bottom is the status bar. On the far left, your location and altitude
above sea level will be listed; the default setting is "Earth, Paris, and 38m."
Next, it tells you the "FOV," i.e. your
field of view
from top to bottom. The default is 60˚. The
following item displays the refresh rate for the animation in frames per second, or FPS. This will
vary depending on the active memory being used by your computer.
Finally, the date and time are displayed in the format "YYYY-MM-DD HH:MM:SS" in 24-hour
time. For example, 2022 January 19 at 4:00 PM would be 2022 01-19 16:00:00. Daylight
Saving Time is automatically run based on your location.
Since this software is displaying
what your local time would be, it is very important that you calibrate this. For the purposes
of this assignment, make sure your computer's time zone is set to Eastern Time (UTC -04:00
during DST, UTC -05:00 in the winter months).
There are dock menus, which pop out from the left side and the bottom. The left menu controls
the broader settings, while the bottom menu controls your viewing settings. Place your mouse
cursor over each of the buttons to get a description of what each button does. A keyboard shortcut
will also be listed in brackets.
Change your location from the default location in Paris.
Access the Location window using
either the shortcut key "F6" (you may have to hold the Function ["Fn"] key at the same time) or
by clicking the top button on the left menu shaped like a compass. The search bar is to the right of
the magnifying glass symbol, where you may type in the name of any town currently listed.
Please find "North Charleston, SC, United States" in the list of cities and click on the name in the
list.
Make sure the coordinates match the following:
2
Latitude: N 32
o
51’ 16.56”
Longitude: W 79
o
58” 29.28”
Altitude 0m.
Check the box on the lower left labeled "Use as default." Close the Location window by clicking
the "
☓
" in the upper right-hand corner.
You can change your view of the sky by dragging it with your mouse. Click and hold the mouse
button on any point, which will allow you to change your view. You may also use the arrows on
your keyboard to alter your viewable sky.
When you select an object in Stellarium, the information for the object appears in the upper left
corner of the screen, but the default setting displays more information than you may need.
Either open the Configuration window using the shortcut key "F2" or by clicking the fifth
button on the left menu shaped like a wrench. Select the Information tab.
Uncheck
the boxes
for the following "Displayed fields:" Right ascension/Declination (J2000), Galactic
coordinates, Hour angle/Declination, Ecliptic coordinates, and Additional Information. Select the
Main tab, then click "Save settings," and close the Configuration window.
The date and time can be adjusted either by accessing the “Date and Time” window using the
shortcut key "F5" or by clicking the second button on the left menu shaped like a clock. You
may change any entry by using the up and down arrow keys. If an entry is highlighted, you
may also type in a new value. Practice changing the date and time to get comfortable using this
feature. Change the date and time to 2020-10-08 at 12:00:00 (noon). If you don't see the Sun
due South-East, i.e. directly above the “SE” in the sky, the clock on your operating system
(Windows, Mac OS X) is not set to the Eastern Time Zone.
When you are in the main window in Stellarium, typing the number "8" is a useful keyboard
shortcut for setting the time. Set the date to 2020-01-01 at midnight, then type "8" in the main
window.
1. How does typing "8" change the date and time?
3
Typing “8” changed the date and time back to what it was previously.
Set the time to 21:00 (9:00 PM) before you move on to the next step. When viewing the sky, you
will notice the ground and the sky, as well as the letter "S" at the horizon representing one of the
cardinal directions, south. Keep an eye on the stars as the time changes.
When using Stellarium, the sky normally moves in real time, but you can control this rate of
motion. You have four buttons on the right side of the bottom menu, which control the rate of
motion: Reverse, Play, Now, and Forward.
Clicking the Reverse or Forward buttons multiple times allows you to speed up the time flow in
either direction, and they can slow down the time flow when they oppose the motion.
The Play button resets the time flow to real time and acts as a Pause button when the sky is
changing in real time.
Finally, the Now button changes the time flow to real time AND changes the date and time to the
present. The Reverse, Play, and Forward buttons all have easy keyboard shortcuts as well: "J",
"K", and "L".
2. From the real-time or Play setting, increase the Forward rate three times. Watch the
southern sky for about 30 seconds and describe what you see. Which direction are the stars
moving?
After increasing the speed forward rate three times the stars began moving to the right or
clockwise. After watching the southern sky for 30 seconds, the turned from night to day, the sun
set and rose again. All of which was moving clockwise.
Instead of altering the rate of time flow, you can move in discrete time steps. Pause the time flow
and reset the time to 21:00 (9 PM). Pay attention to the time and date as you click the "-" and "="
keys. You can also change the time at different rates by holding down the "Ctrl" key at the same
time.
Mac users:
For the keyboard shortcuts listed below, use Command (
⌘
) instead of Control
("Ctrl").
4
3.
Record how the date and time changes when using each of the following keyboard
shortcuts:
a)
– when you press this key – the moon moves to the right and the time stays the same, but the
date jumps backwards a day.
b)
= when you press this key, the moon jumps left and the time stays the same, but the dates
jumps forward a day.
c)
[ when you press this key, the time stays the same, but the date jumps backwards a week or 7
days.
d)
] when you press this key, the time stays the same, but the date jumps forward a week or 7
days.
e)
Ctrl – when you press this key the time jumps backwards an hour.
f)
Ctrl = when you press this key the time jumps forward an hour.
While looking at the sky as you would see it from North Charleston, you can select any of the
points of light in your field of view to see some information about the object. Choose a bright,
unlabeled
point of light in the sky and click the mouse button to select it.
4. Write down the name of the object (only the first part listed), its magnitude (only the
first number listed), and its distance from Earth rounded to one decimal place. Do not
forget the distance units.
Magnitude: 1.00 (reduced to 1.32 by 2.44 Airmasses)
Distance: 533.75 ly
Something that you will have noticed is that it is often hard to keep track of the stars because the
Sun comes up. Fortunately, Stellarium allows you to remove the effects of daylight hitting the
atmosphere. On the bottom menu, one of the highlighted icons looks like a cloud obscuring light.
Clicking this button or typing the shortcut, "A", removes the atmosphere and allows you to see
the stars hidden by scattered sunlight.
5
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Related Questions
Suppose a spectral line from an object in space was shifted from 5007.0 to 5100.0 Angstroms. What can we tell about this object?
A) It is a star.
B) It is very cold.
C) It is blueshifted, hence coming towards us.
D) Its radial velocity is positive, meaning it is moving away from us.
E) It is a planet in a distant galaxy.
F) It is an exoplanet.
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Question A3
The figure below shows the Hertzsprung-Russell diagram (HRD) for two star clusters using data
from the Gaia mission (Gaia Data Release 2, A&A 2018). The absolute magnitude and colour
index are defined using a Gaia defined photometric system.
MG
-2
0-
2
4-
16
Open Cluster M 67
8-
Globular Cluster 47 Tuc
0.0
0.5
1.0
1.5
2.0
2.5
GBP - GRP
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clusters.
b) Explain the form of the HRD for the two clusters, indicating on a sketch the main features.
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required.
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4um
Fig. 17.2
i) The diameter of the Kupffer cell in the image is 9.1 cm. Assuming it is spherical, caloulate the actual volume
of this cell.
Give your answer to four significant figures. Show your working
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Group of answer choices
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Very distant galaxies are more likely to contain planets than the Milky Way is, so we have a better chance of detecting life in those galaxies than we do in our own galaxy.
Since the light from these galaxies took so long to reach us, we're seeing them as they were when the universe was very young.
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(subject: astronomy)
1. When do you say a star is very hot compared to the red.
2. are stars of equal size? explain your answer
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No need to solve. Just formulate all the equation that can be seen in the diagram. Examples are
Bx= B cos (- theta 1)
By= B sin (- theta 2 )
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Tutorial
A molecular cloud has a temperature of 46 K and an HI cloud has a temperature of 135 K. What are their wavelengths of maximum intensity?
What frequency do these correspond to?
In what region of the electromagnetic spectrum can the radiation from these clouds be found?
Part 1 of 3
We can use Wien's Law to determine the wavelength of maximum intensity in nanometers for the molecular cloud.
2.90 x 106
Amc
Amc
Amc
XHI
^HI
=
AHI
=
We can use Wien's Law again to determine the wavelength of maximum intensity in nanometers for the HI cloud.
2.90 x 106
II
=
K
nm
=
μm
K
nm
um
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1. The relative velocities of four stars are shown in the figure below with arrows.
If an astronomer were to study the light from these four stars, in which star would the astronomer see greatest redshift of its light spectra? Hint: Think Doppler Effect
A. star 1B. star 2C. star 3D. star 4
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Please answer within 90 minutes.
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4.
on
the
ONLY
next page
compare
differences
in
and luminosity (more or
Refer to the figure
following questions.
temperature (hotter or cooler)
less luminous) as determined from the diagram. In other
words, consider only what you know about relationships
between temperature versus luminosity, diameter
luminosity, or color versus temperature relationships.
make
NOT
*IMPORTANT NOTE: DO
stars' masses or stage of life
answer.
any
versus
reference
to the
for your
as a reason
a) WOLF 28 and PROCYON have roughly the same
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(Explain which property of the star supports your
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Which star is smaller in diameter?
(Explain which
property of the star supports your reasoning.
Review…
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The stars with the most prominent hydrogen absorption lines are O stars.
K stars have many more spectral lines than B stars.
Heavy elements generally have fewer spectral lines than light elements.
An absorption line is produced when a cooler gas absorbs light from a bright
background continuum light source.
Emission lines are produced when electrons jump from low energy levels to high
ones.
The longest wavelength Hydrogen Balmer line is red.
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2:54 PM Fri 23 Apr
* ni 26%
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blob:https://web.whatsapp.com/d4009cff-87ec-4851-8d8a-2f11269ecb47
G Identify the names of the four major arms of Milky way galaxy : - Google S...
This section contains 6 multiple choice questions. There can be more than one correct
answer. Each question is of 3 marks. For an incorrect answer, 1 mark will be deducted.
However, a partial mark will be awarded for every correct option unless no incorrect
option has been chosen.
Multi correct :
Q.1
A human eye is most sensitive to that wavelength( Am) at which the energy distribution of solar
radiation shows the maximum.
A. Apply Wien's Displacement law to calculate Am . Take the sun's surface temperature as
5800 K , and wein's constant, b = 0.29cm.K.
B. Taking the average surface temperature of the earth as approximately 290K, calculate
the wavelength at which it radiates most.
= 5000 A°
a) For part A, Am
b) For part B, 2,m would be in infrared region of electromagnetic spectrum
c) For part…
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B9
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Problem 4. Stellar Temperature, Color, and Size
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i) which star is actually more luminous?
ii) Betelgeuse appears reddish while Rigel appears bluish white. Which star is larger and why?
b) (Palen, et. al., 2nd, Problem 46) Sirius is actually a binary pair of two A-type stars. The brighter and fainter of the pair is called the Dog Star and Pup Star, respectively (they are in the constellation Canis Major). The Dog Star is 6,000 times brighter than the Pup Star even though both stars are the same distance from us. Compare the
i) temperature
ii) luminosities
iii) sizes (radii)
of these two stars. (CALCULATE using the principles of brightness and the Stefan-Boltzmann law, do not look up the answers! HINT: Star letter type is a measure of temperature)
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- Suppose a spectral line from an object in space was shifted from 5007.0 to 5100.0 Angstroms. What can we tell about this object? A) It is a star. B) It is very cold. C) It is blueshifted, hence coming towards us. D) Its radial velocity is positive, meaning it is moving away from us. E) It is a planet in a distant galaxy. F) It is an exoplanet.arrow_forwardQuestion A3 The figure below shows the Hertzsprung-Russell diagram (HRD) for two star clusters using data from the Gaia mission (Gaia Data Release 2, A&A 2018). The absolute magnitude and colour index are defined using a Gaia defined photometric system. MG -2 0- 2 4- 16 Open Cluster M 67 8- Globular Cluster 47 Tuc 0.0 0.5 1.0 1.5 2.0 2.5 GBP - GRP a) Briefly describe the morphological (i.e., shape related) properties of open and globular clusters. b) Explain the form of the HRD for the two clusters, indicating on a sketch the main features. c) Explain how the age of a star cluster can be determined, making clear the assumptions required. d) From the figure what can you infer about the ages of the two clusters shown? Explain your reasoning.arrow_forwardCosmic Microwave Background 8. The Cosmic Microwave Background (CMB) acts as a perfect black body whose energy spectrum(energy density per unit volume per unit frequency) is given by the expression : (image attached)arrow_forward
- Downloads/OCR ExamBulider e 4um Fig. 17.2 i) The diameter of the Kupffer cell in the image is 9.1 cm. Assuming it is spherical, caloulate the actual volume of this cell. Give your answer to four significant figures. Show your workingarrow_forwardI don't understand how to solve for (d) and need some help understanding the equation.arrow_forwardAnalyze the multi-wavelength images below and answer the few questions that follows up : 1. Where do you see the higher energy phenomena? What are they? Are they visible in any image? Why?2. Where are the young stars? What colour do they have? Are they visible in any image? Why?3. Where are the old stars? What colour do they have? Are they visible in any image? Why?arrow_forward
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