Stellarium Introduction
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S
TELLARIUM
: I
NTRODUCTION
1.
Launch the program.
The program has two navigation panels which appear when you mouse over: one on the left
and another at the bottom of the screen. Move your mouse over each tool so that you can familiarize yourself with the menu.
There are also several hotkeys which turn on and off certain features. There is a list of Stellarium shortcuts in the Week 1 Module which you may want to reference for future labs.
If you click on an astronomical object, an information panel shows on the left. You can get rid of this by right-clicking.
2.
From the left panel, select the Location Window (F6) and search for Columbia (Missouri)
in the search bar (the one with the magnifying glass). Ensure that the red arrow on the world map moves to Columbia. Click the box in the lower left to make this your default location. Close this window. You should see your location listed in the lower left of the viewing window.
3.
Let us begin by pretending the Earth does not have an atmosphere so that we can see the stars even
during the day. To do this, hit the "A" key to turn off/on the atmosphere.
4.
Change your viewing direction by clicking on the ground and dragging. Orient your view to the East and observe how the stars move with respect to your horizon. You will want to speed time up. To do
this, click "L"
three times
. (You can return to normal speed at any time by hitting the "K" key.)
5.
Describe the motion you observe for each cardinal direction. EAST – SOUTH – WEST – NORTH – 6.
Open the Location Window (F6) and change your location to Sunbury, Australia
. Repeat the observations. Describe the motion of the stars in each direction.
EAST – SOUTH – WEST – NORTH – How has the movement of the stars changed?
7.
Open the Location Window (F6) and change your location to Beni, Congo
. Repeat the observations. Describe the motion of the stars in each direction.
EAST – SOUTH – WEST – NORTH – How has the movement of the stars changed?
8.
Open the Location Window (F6) and change your location back to Columbia (Missouri)
by clicking on
the “Return to default location” button. You should see “Earth, Columbia (Missouri)” in the lower left corner when you return to the main screen.
9.
Orient your view to the North and find Polaris (The North Star). You may want to click on the ground
and drag it downward. Polaris is directly above the North direction, and it should not be moving like all the other stars. Click on Polaris. This will bring up lots of information about the star in the upper left of your screen. Find the data entry labeled: "Az/Alt". This is the azimuth and altitude of Polaris. Record the altitude below. Just give the angle in degrees and minutes.
Altitude of Polaris: _____________________
Determine the latitude of Columbia, MO as well. This can be found in the Location Window (F6).
Latitude of Columbia, MO: _________________
Compare the two numbers. They should match within a degree of each other. This will hold true for any location in the northern hemisphere and is historically a very useful navigational tool. 10.
Hit the “7” key on the keyboard to stop time. We can observe the sky at any time by opening the Date/Time Window from the left navigation panel or by hitting F5. Note that the clock is in 24-hour format. Change the date to 2021-1-20
and the time to 19:00:00
(this is 7pm on January 20). Move the Date/Time window to the lower right of your screen so that it is out of the way but still visible.
11.
Open the Search Window by clicking on the magnifying glass icon in the left navigation panel or by hitting F3. Search for Sirius
. Once the star is selected, hit the spacebar to keep the object centered.
12.
In the chart on the next page, record its azimuth and altitude every hour
through 2am (2:00:00). Record only the degrees
; you can ignore the minutes and seconds for this exercise. Do not use the fast forward time this time. Instead, advance time incrementally by one hour at a time. To do this, click on the clock to select it again, and click the small arrow above the hour position.
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Plz solve within 30min I vill give definitely upvote and vill positive feedback thank you sir
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If theta dot is the slew rate, what would be the maximum slew rate? How would you differentiate theta dot to get theta double dot?
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BINARY STARS
31
Problem 5. Binary star systems: Center of mass. (Palen, et. al. Chp. 10 1st Ed.
Problem 65)
d2
m, = 3m,
The center of mass is where
the fulcrum of a balance must be.
m2
%3D
dz = 3d,
FIGURE 10.15 The center of mass of two objects is the "balance" point on a line joining the
centers of two masses.
Study Figure 10.15 in the text (1st ed.). Where would the center of mass be located
if
а) т — т?
b) M¡ = 2m,?
c) 2m2= 3m,?
11:50 PM
e Type here to search
3/4/2021
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Problem 3. Brightness and Luminosity
31
The brightness or flux intensity of a star at an observer's location may be
determined by measuring the rate at which its light enters the aperture of an
observing instrument (this is referred to as photometry). We will call this "" (with
units [Energy/time/Area] or [Watts/Area]). Imagine a sphere of radius, d (labeled
"p" in the figure below), equal to the star's distance from the observer's location,
at which the star is at the center (see the figure below). ALL of the star's light
passes through the surface area of this sphere but only a small fraction passes
through the instrument aperture. The fraction of the star's rate of light energy
emission measured by the instrument is…
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b Answered: A ball thro x C A ball thrown horizont x C A ball thrown horizont X
lc.lib.jmu.edu/res/jmu/constacx/HW3-P2-PHYS240-FA18.problem?symb=uploaded%2fjmu%2f41283831cd70463c3jmul1%2fdefault_1536805168%2esequence____...
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Course Contents >>> >> Homework 3 » HW3-P2-PHYS240.problem
A ball thrown horizontally at 45 m/s travels a horizontal distance of 162 m before hitting the ground. From what height (in m) was the ball thrown using 9.80 m/s² as the local acceleration due to gravity?
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Schedule | Central Mich
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What is the wavelength of an electron with a velocity of 10’ m/s?
7.28 x 10-11 m
ni
an
EA
LATI
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What is the wavelength of a 50 gram rock moving
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3.32 x 1034 m
Chi
you
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A) The pressure that balances gravity in a white dwarf is called degenerate electron pressure.
B) The power source of white dwarfs is left-over heat.
C) White dwarfs cool slowly because they are small and eventually fade-out to become black dwarfs.
D) White dwarfs with mass greater than 1.4 times the Sun's mass cannot exist.
E) Stars with a mass like the Sun will end up as a white dwarf star.
F) White dwarfs are less dense than red giants.
G) White dwarfs are the coolest main sequence stars.
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to collapse in "free-tall to form a new star is half
the time it would take for an object to orbit the star
on an extremely elliptical orbit with a semimajor
axis of 53,000 AU (half the 106.000 AU radius).
Part A
Use Kepler's third law to find the collapse time, assuming the star has the same mass as the Sun.
Express your answer in years to two significant figures.
VE ΑΣΦΑ
t=
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years
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2. How many light years in 1 pc?
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Section I fishbowl discussion qu X
The Metamorphosis Section I by x
/document/d/1yMSODoiaY46JaL-uTnNJOPFgkVnR1Hp3qgzKCVTaiu4/edit
6 What kind of party...
ion questions D O
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BIUA
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Calibri
11
E E E E
2
The Metamorphosis Section I Fishbowl Discussion Questions
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(a)
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(c)
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mmmmmm
0.0001 nm 0.01 nm
Gamma rays
400 nm
Increasing energy
X-rays
Increasing wavelength
10 nm 1000 nm 0.01 cm
Ultra-
violet
Infrared
Visible light
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600 nm
Figure 2: Electromagnetic spectrum
1 cm
1m
Radio waves
Radar TV FM
700 nm
100 m
AM
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1,0 kg
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A fish swimming in a horizontal plane has velocity v = (4.00 î + 1.00 j) m/s at a point in the ocean where the position relative to a certain rock is F = (16.0 i - 3.00 j) m.
After the fish swims with constant acceleration for 17.0 s, its velocity is v = (21.0 î - 3.00 j) m/s.
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a, =
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a, =
m/s2
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y =
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° counterclockwise from the +x-axis
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- E A X X Math M Inbo b Last Class N Netf + Prob Logir M Inbo 4 Good #3 Grou Mail y! CVX EHL 4 fre ET Wha G neve docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit M AST1002001FALL2017PS7 ☆ Request edit access Share File Edit View Tools Help BINARY STARS 31 Problem 5. Binary star systems: Center of mass. (Palen, et. al. Chp. 10 1st Ed. Problem 65) d2 m, = 3m, The center of mass is where the fulcrum of a balance must be. m2 %3D dz = 3d, FIGURE 10.15 The center of mass of two objects is the "balance" point on a line joining the centers of two masses. Study Figure 10.15 in the text (1st ed.). Where would the center of mass be located if а) т — т? b) M¡ = 2m,? c) 2m2= 3m,? 11:50 PM e Type here to search 3/4/2021 + (8) IIarrow_forwardE A X M Inbo b Last Class N Netf + Prob Logir | X Math M Inbo Good #3 Mail y! CVX ET Wha 4 Grou EHL 4 fre G neve docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit M AST1002001FALL2017PS7 ☆ A Request edit access Share File Edit View Tools Help Problem 3. Brightness and Luminosity 31 The brightness or flux intensity of a star at an observer's location may be determined by measuring the rate at which its light enters the aperture of an observing instrument (this is referred to as photometry). We will call this "" (with units [Energy/time/Area] or [Watts/Area]). Imagine a sphere of radius, d (labeled "p" in the figure below), equal to the star's distance from the observer's location, at which the star is at the center (see the figure below). ALL of the star's light passes through the surface area of this sphere but only a small fraction passes through the instrument aperture. The fraction of the star's rate of light energy emission measured by the instrument is…arrow_forwardLON-CAPA HW3-P2- X - с b Answered: A ball thro x C A ball thrown horizont x C A ball thrown horizont X lc.lib.jmu.edu/res/jmu/constacx/HW3-P2-PHYS240-FA18.problem?symb=uploaded%2fjmu%2f41283831cd70463c3jmul1%2fdefault_1536805168%2esequence____... M Gmail Jeffrey Sabol ▾ (Student) Main Menu Contents Grades YouTube Maps Submit Answer Tries 0/10 Post Discussion Translate PHYS240_0001_FA22 Day 08 Problems: Uni x 2.3 Homework-Limit X MacBook Pro Feedback Course Contents >>> >> Homework 3 » HW3-P2-PHYS240.problem A ball thrown horizontally at 45 m/s travels a horizontal distance of 162 m before hitting the ground. From what height (in m) was the ball thrown using 9.80 m/s² as the local acceleration due to gravity? Timer ii Handshake Notes 34 x + D 0 j Update Messages Courses Help Logout Evaluate Print Inf Send Feedbacarrow_forward
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