RanaAditya_Lab3
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M
ONTGOMERY
C
OLLEGE
– R
OCKVILLE
A
STRONOMY
101 ASTR101
Laboratory 3 – Mapping the Night
Sky
1
Name: Aditya Rana
Ever tried to give someone directions to a friend's house without knowing the exact
address? It’s hard! Just as buildings have addresses to help us find them,
astronomers need ways to locate things in the sky. Ideally, there should be a precise
way to map the sky, just as we have a map of the surface of the Earth.
To locate any point on the surface of the Earth, we specify the point’s
LATITUDE
and
LONGITUDE
, two angles that measure a spot's position relative to the center of
the Earth. For example, Rockville (at least the center of it) is located at
39º North
,
and
77º West
. Similarly, we need a way to tell other astronomers where to look for
things in the sky. We can’t just say “Look to the left of that bright red star and then
go up a little.” In this assignment, we’ll study the two ways of locating objects in the
sky using angles – one called
Altitude & Azimuth (Alt/Az)
, and the other called
Right Ascension & Declination (RA/Dec)
- and their relative advantages &
disadvantages.
PART A
Start
Stellarium
. Make sure your location is
Rockville
. If it is not, open the
Location
window, enter
Rockville
in the search box and then click on
Rockville,
United States
, and then close the
Location
Window. Turn off the Atmosphere and
Fog (if they're on), by pressing the
A
and
F
keys (sky should be dark). Put the
horizon at the center of the screen by dragging it until it's at the center. It doesn't
matter which part of the horizon – N, S, E or W, you choose. Pick a star that is as
close to the horizon as possible. Click on it. Information on your star will appear in
the
upper left-hand corner
of the screen.
Use red font for your answers.
What is the common name of your
star?
Procyon
In the information (upper left-hand corner), look for the line that starts
Az/Alt
.
Az/Alt
stands for
Azimuth/Altitude
, and the numbers on this line list the angles
1 Last edit Spring 2022.
1
ASTR101
L
ABORATORY
3
that are the star's Azimuth and Altitude, as discussed in class. The first number
listed is the Azimuth, and the second number, after the slash, is the Altitude.
What are the Azimuth and Altitude of your star?
ROUND OFF ALL YOUR AZIMUTH
AND ALTITUDE READINGS TO THE NEAREST DEGREE – IN OTHER WORDS,
IGNORE EVERYTHING AFTER THE ° SYMBOL!
Azimuth
:
+272
Altitude
:
+4
Try a few other stars along the horizon. Click on them. Look at their altitudes.
Compare the answers to what you saw for your first star. Do you notice a pattern?
What is the approximate value of
altitude
(in degrees)
for any star on
the horizon?
+3-4
Now find a star that is
straight above
one of the stars you just chose. In other
words, look a little higher in the sky. Click on the new star. Note its altitude and
azimuth, and compare them to the values for the stars on the horizon. One of the
numbers will have changed, and the other will be (approximately) unchanged.
As you move the cursor
straight up
from the horizon (in other words, as
you look up from the horizon, toward
the zenith), which angle changes,
Altitude or Azimuth?
The Altitude Changes
Zoom out
and re-center the sky until you are looking at the entire sky at once.
Click as close as you can to the zenith (the point at the center of the screen).
Remember, the zenith is the point directly over your head in the sky.
What is the value of altitude (in
degrees) at the zenith?
90
Altitude is an angle that tells you where a star is above the horizon. Picture two rays
coming from your head – one pointing at the horizon directly below the star, and the
other pointing at the star you're looking at. The angle between those rays is the
altitude of a star.
Click the cursor on a star that is
below
the horizon – in other words, click on the
ground. Notice the value of the altitude here.
How can you tell by looking at a star’s
Because the value of the altitude is in
2
ASTR101
L
ABORATORY
3
altitude whether it is above or below
the horizon?
negative
.
Go back and click on a few more stars on the horizon.
As you click
left or right along the
horizon
, which angle changes, Altitude
or Azimuth?
The Azimuth changes
Click around the entire horizon (you may have to move the horizon by grabbing it
with the cursor and dragging it), and watch the Azimuth change.
Drag the sky around so you're looking at the
Northern
horizon. Click on various
places on the horizon just to the left and right of
North
, and look at the values of
altitude and azimuth for various points on the horizon.
What is the maximum value of
azimuth?
360
What is the azimuth of
E?
90
What is the azimuth of
W?
270
What is the azimuth of
S?
180
What is the azimuth of
NW?
315
Azimuth measures the angle along the horizon in degrees, to your chosen star,
starting at North and going clockwise.
Find the star Polaris, using
Stellarium's
Search
window (or by using
CTRL-F
or the
F3
key).
What are the altitude and azimuth of
the star
Polaris
?
Azimuth
:
359
Altitude:
38
What is the latitude here in ROCKVILLE, where you are observing from? (To find your
latitude, open the
Location
window – your latitude and longitude are listed there)
Latitude Rockville:
39
3
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L
ABORATORY
3
Comparing the answers to the previous
two questions, what might you guess is
the relationship between an observer’s
latitude
and the
altitude
of Polaris
above his or her horizon?
The altitude of Polaris is always same
to the observer’s latitude.
Stellarium
can superimpose a grid on the sky that allows you to easily measure
Altitude and Azimuth. To show this grid, press the “
Z
” button on your keyboard (or
go to the toolbar at the bottom of the screen and click on
Azimuthal grid)
. The
lines in the grid that run parallel to the horizon are lines of altitude, measuring from
the horizon to the zenith, and the lines that are perpendicular to the horizon, and
which all meet at the zenith like the spokes of a wheel, are lines of azimuth,
measuring along the horizon, from North. The grid lines are labeled, in degrees
where they hit the edge of the screen.
Set the time for
8 PM
tonight by changing the time in the
Date/Time
window.
Label the brightest stars by opening the
View
window and putting a check next to
Stars
(in the
Sky
sub-menu). Also, move the slider next to
Labels and Markers
to
about half way from the left. Close the
View
window.
Now search for the star named
Dubhe.
You should see that it is located in the bowl
of the Big Dipper in the constellation
Ursa Major
.
Don't forget, if you want to see
the constellation outlines and names on the screen, press
C
and then
V
.
What is Dubhe’s Altitude and Azimuth
at 8 PM tonight? (
Remember, if you
click on a star, its data will be
shown onscreen.)
Azimuth
:
333
Altitude
:
22
Change your location to
Pueblo, CO
(
Lat=38º N, Lon=104º W
) in the
Location
window by entering
Pueblo
in the search box and then scrolling down until you find
Pueblo, United States of America
in the resulting list and clicking on it.
Stellarium will put you at 6pm local time (18:00), the same as 8pm in Rockville.
Before answering the following,
change the time to 8 PM
in Pueblo (20:00)!
Find Dubhe's altitude and azimuth in
Pueblo.
Azimuth
:
334
Altitude:
20
Are Dubhe's altitude and azimuth
similar in Pueblo and Rockville at 8PM
Yes
4
ASTR101
L
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3
in each location?
They should be similar! Explain why.
Because the change in latitude was
insignificant to affect the viewers
observation of dubhe
Change your location to
Fairbanks, AL
(
Lat=64º N, Lon=147º W
) in the
Location
window by entering
Fairbanks
in the search box and then scrolling down
until you find
Fairbanks, United States of America
in the resulting list and
clicking on it. Before answering the following,
change the time to 8 PM
in
Fairbanks (20:00)!
Find Dubhe's altitude and azimuth in
Fairbanks.
Azimuth
:
318
Altitude:
47
Are Dubhe's altitude and azimuth
similar in Fairbanks and Rockville at
8PM?
NO
They should be different! Explain why
your results for Pueblo and Fairbanks
are different.
Because of the location change the
latitude value is significantly different
which affects the observers view
Change your location back to
Rockville
, and the date back to today's date, at
9
PM
.
Back in ROCKVILLE, what is Dubhe’s
altitude and azimuth at
9 PM
?
Azimuth
:
339
Altitude
:
17
Do a star's altitude and azimuth stay
constant as the night goes on?
(Compare the Alt/Az for Dubhe at 9 PM
with the Alt/Az you found at 8 PM in
Rockville.)
It does not
What is Polaris' altitude and azimuth at
8 PM
?
Azimuth
:
0
Altitude
:
38
What about at
9 PM
?
Azimuth
:
0
Altitude
:
38
You should find that the Alt/Az of
Polaris does NOT change. Explain why
Dubhe behaves differently from Polaris.
The reason why there is no difference
in Polaris’s values is because it is very
close to the celestial pole, where as the
other stars are not and the movement
of the earth affects their values.
5
ASTR101
L
ABORATORY
3
If someone told you they saw a satellite at
85
degrees altitude, where would you
look (check one)?
Near the horizon
Near the Zenith
x
Halfway up the sky
None of the above
If you wanted to tell someone to look
at a star halfway up the sky in the
Southeast
, what
Alt
and
Az
would you
give?
Azimuth:
135
Altitude:
45
PART B
As we have seen, altitude and azimuth have one large drawback - they are
observer dependent
– they change, depending on both
where
the observer is,
and
what time
he or she is observing. We need a set of coordinates that are
observer
in
dependent, that never change, like Latitude and Longitude on the Earth!
The coordinates we have developed that fit the bill are called
Right Ascension
and
Declination
, together known as the
Equatorial System
.
Right Ascension and Declination (
RA
and
Dec
), are the two numbers we use to
specify a star’s location, using a grid fixed on the sky. To display that grid, first turn
off the
Azimuthal
grid by pressing the
Z
key, and turn on the Equatorial grid by
pressing the
E
key. You can also turn these grids on and off using their buttons in
the
toolbar
at the bottom of the screen. Drag the sky around and zoom out until
the Southern horizon is at the bottom of the screen and you can see the whole sky
at once.
You should see a different grid pasted over the sky – this one in blue. The lines that
shoot out like curved spokes from the
North Celestial Pole
are lines of
Right
Ascension
. The circular lines perpendicular to these Right Ascension lines are lines
of
Declination
. Again, the lines are labeled with their units at the edge of the
screen. These lines are the grid that we use to measure fixed address locations in
the sky.
6
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The Right Ascension and Declination of any star's position are listed in the
information that appears when you click on that star.
Click on any star. The information about that star appears in the upper left-hand
corner of the screen. Look for the line that reads
RA/DE (J2000)
. The two sets of
numbers separated by a slash are the star's Right Ascension and Declination. Let's
look at
Declination
first.
What units is declination measured in?
degrees
Press the
“.” (the period)
key on your keyboard. This will highlight the
Celestial
Equator
in brighter blue. Pick a star lying right along the Celestial Equator. Click on
it. Look at the star's Declination. Do this for a few more stars along the Celestial
Equator. (If you can’t see it because it’s the same color, toggle the equatorial grid
on and off with the E key.)
What is the Declination anywhere on
the Celestial Equator?
0
Make sure you're looking at the whole sky by
zooming out
and centering the sky
on the screen. Click on various stars and watch the information that appears for
them. Notice that the Right Ascension (RA) and Declination (Dec) change in various
places in the sky. Try to find the place where Declination reaches its maximum
value.
What is the maximum value of
declination?
90
What is the name of the bright star
almost exactly at the point where
declination reaches its maximum
value?
Polaris
What angle does declination measure?
The angle from the celestial equator
Now let’s look at the
Right Ascension
lines. Again, these are the lines that circle
the celestial sphere but run through the north and south celestial poles.
Unlike Declination, which is measured in degrees (and fractions of a degree called
arc-minutes and arc-seconds), Right Ascension is measured in a different unit. Click
on a few stars and look at their Right Ascension values.
7
ASTR101
L
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What are the units RA is measured in?
(Hint: look at the letters that appear in
the RA scale.)
In time
Click on various stars along the Celestial Equator (the brighter blue line) and note
their Right Ascension. Do you see a pattern? Keep clicking on stars and try to find
the maximum value of RA. You may have to let some time pass to click all the way
along the entire Celestial Equator.
What is the maximum value of RA
(before it starts over again at zero)?
23h 59m
What is the exact RA of Polaris? (Click
on Polaris to see information.)
2h33m09.64s
Center the whole sky on the screen, and click on a star as close as possible to the
zenith to estimate the RA and Dec coordinates of the zenith itself. Don't forget to
write the units for each measurement below!
Zenith RA:
19h
Zenith
Declination:
41
Now change the time to
1 hour
later. Again, click on a star as close as possible to
the zenith to estimate the new RA and Dec coordinates of the zenith.
DO NOT CLICK ON THE SAME STAR
. Click in the center of the circle. Your zenith
is always the center of the circle.
IF YOU ARE GETTING THE SAME RA EACH
TIME, YOU’RE DOING IT WRONG
.
Zenith RA:
20h
Zenith
Declination:
41
What would you guess the RA and Dec coordinates of the zenith would be
six
more
hours later?
Zenith RA:
2h
Zenith
Declination:
41
The answers to the previous questions should help you understand why RA is
measured in hours (and minutes and seconds). Each hour that passes causes one
hour of Right Ascension to pass by any point in the sky.
8
ASTR101
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Right Ascension and Declination, or the Equatorial system is a much more useful
way to locate stars and objects in the sky than Altitude and Azimuth. To see why in
another way, turn both grids on at once by pressing
Z
and
E
until you see both grids
at the same time. Press
L three
times to let time go by at
1000
times normal
speed and watch the stars move across the sky.
Do the stars stay fixed relative to the Alt/Az grid as time
passes?
no
If we use Altitude & Azimuth to measure a star's position,
would the star's Altitude and Azimuth stay the same as the
night went on?
no
Do the stars stay fixed relative to the blue Equatorial grid as
time passes?
yes
If we use Right Ascension and Declination to measure a star's
position, would the star's RA and Dec stay the same as the
night went on?
yes
Now you can see why we use Right Ascension and Declination as our “address” in
the sky. RA and Dec do not change, regardless of where the observer is on Earth, or
what time of day or night it is, or what day of the year it is.
PART C
We can now give every spot in the sky a unique address that won't ever change,
using Right Ascension and Declination. This applies not just to stars, but to “Deep
Sky” objects, like nebulae, galaxies, and star clusters. Practice looking up some of
these addresses by filling in the
Deep Sky Address Table
on the table below.
Find each object by either opening the
Search
window from the menu, or by typing
CTRL-F
or
F3
. Once the object is selected and in the center of the screen (you may
have to hide the ground by pressing “
G
” to see some of the objects), then zoom in
until you can see each of the objects. The object's information, including its
RA
and
Dec
address, will be displayed in the upper left-hand corner of the screen. Just list
the degrees and arcminutes for Declination, and the hours and minutes for Right
Ascension.
Deep Sky Object Name
RA
Dec
Andromeda Galaxy (M31)
0h42m
41
Orion Nebula (M42)
5h35m
-5
Lagoon Nebula (M8)
18h03m
-24
Ring Nebula (M57)
18h53m
33
Whirlpool Galaxy (M51)
13h29m
47
9
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In the space below, write a brief conclusion explaining what the advantages and
disadvantages are of using Altitude & Azimuth or Right Ascension & Declination,
and what you learned about them in this exercise.
The benefits of using the altitude and azimuth is that although it might give the
accurate position for the current time the values change quite frequently. That's
why the use of right ascension and declination is better because the values are
fixed on the Equatorial map, and they do not change.
10
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