magnitudes lab (Complete)
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Sam Houston State University *
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1403
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Astronomy
Date
Dec 6, 2023
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THIS LAB EXERCISE IS WORTH 2.5 POINTS
In astronomy, it’s vitally important to be able to measure the amount of light we see from a star. Without knowing
how bright a star really is, we can’t accurately determine many of its other properties. Unfortunately, eyeballing a
star in the sky is no better than walking into a darkened room with an unknown light source and trying to figure
out how it compares to another light source.
The ancient astronomers knew how bright stars APPEARED, and so they created a system of
magnitudes
to keep
track of this appearance. Later, when we understood more about the actual amount of light coming from the stars,
we adjusted the magnitude system to reflect this information.
Stars now have two major magnitude designations –
absolute
and
apparent
.
Which quantity – absolute or apparent – do you think tells you something about the
actual
amount of light from a
star?
Explain:
Absolute tells you about the actual amount of light coming from a star.
If you were to look at two light bulbs and gauge their brightness from your location in your house, are you gauging
the absolute or apparent magnitudes of the bulbs?
Explain:
I think you would be gauging the apparent magnitudes of the bulb, not the actual absolute magnitude.
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The magnitude system in astronomy is the cause of many headaches because the scale seems to go in the wrong
direction. Large absolute magnitudes represent objects that have low luminosities. Small (and negative) absolute
magnitudes represent objects with high luminosities.
One way to think about this peculiar system is to compare it to a golf scoreboard, where the number relative to
shooting ‘par’ is often displayed. A golfer who completes a round with fewer strokes than another is a better
(brighter) golfer. Consider the following scoreboard:
Which golfer(s) had the WORST round?
I.Poulter, who has +2.
Which golfer(s) had the BEST round?
P.Mickelson and J.Kelly who both have -5.
Does a positive number correspond to a better or worse golfer?
A positive number corresponds to a worse golfer. The more negative a number is, the better.
Now consider the following list of APPARENT magnitudes:
Star A
+1
Star B
0
Star C
-3
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Which star appears brightest in our sky? _
Star
C
_
Explain:
It has a larger negative M, meaning it is much more luminous than both Stars B and A.
Which star appears faintest in our sky? _
Star A
__ Explain:
Star A’s apparent magnitude is in the positive, meaning that it’s more faint.
Can you tell which of the stars in the above list is ACTUALLY faintest? _____ Explain:
no, you can’t tell which of the stars would be the faintest by just having the apparent magnitudes. You’ll need to
have the absolute magnitudes to help tell you which one is actually the faintest. Once you get the absolute
magnitudes, whichever magnitude has the biggest negative will be the most luminous, while the opposite end will
be the least faintest.
The appearance at a specially designated distance gives you information about the actual brightness of the object.
This is related to the
absolute
magnitude. There is nothing inherently special about this designated standard
distance except that it is what humans decided was a good reference point.
In astronomy, the absolute magnitude is what the star WOULD look like (its apparent magnitude) if the star were
viewed from a distance of 10 parsecs (32.6 light years).
Look at the table of stars again. In addition to their apparent magnitudes, we have listed their absolute
magnitudes:
Star
Apparent magnitude
Absolute Magnitude
Star A
+1
0
Star B
0
+4
Star C
-3
+1
Which star has the smallest luminosity? ___
Star
A
____ Largest? _____
Star
C
_____
Which star(s) are FARTHER AWAY than 10 parsecs? ______
A
______ Explain your reasoning:
Star A is further away because Star B is exactly 10 parsecs (if it’s 0, then it’s exactly 10), and Star C would be much
closer than Star A.
Why does the star that APPEARS faintest look fainter than the other stars?
Explain your reasoning:
The star appears less fainter than the other stars because it’s much closer (more than 10 pc) than the other stars.
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THE MAGNITUDE SCALE
The stellar magnitude scale is such that FIVE steps in magnitude represent a factor of 100 in intensity. A single step
in magnitude represents a factor of 2.512 in intensity. Thus if Star A has an apparent magnitude of 1, we receive
2.512 times as much light from it as we do from Star B, which has an apparent magnitude of 2.
In addition, a star with an
absolute
magnitude of 1 has a
luminosity
that is 2.512 times greater than a star with an
absolute magnitude of 2.
The apparent magnitude of the Sun as seen from 10 parsecs away is 4.74. This is also the value of its absolute
magnitude because 10 parsecs is the standard reference distance. The absolute magnitude of the star Sirius is
-1.44 (it’s a negative quantity).
Which of the following is true?
a.
the Sun is about 6 times as luminous as Sirius
b.
Sirius is about 6 times as luminous as the Sun
c.
the Sun is over 100 times as luminous as Sirius
d.
Sirius is over 100 times as luminous as the Sun
e.
there is no way to compare the luminosities of these objects without more information
Fully justify your answer:
Since the apparent magnitude of the Sun can be seen from 10 parsecs away, with the information provided the
magnitude of Star A would have to be at least 100 (due to the 5 steps). We can assume that it’s over 100, due to
the fact that its luminosity is 2.512.
Return now to the Excel table you created in the lab activity on parallax in Unit 1. Within Excel, select the entire
data set and sort by vmag (apparent magnitude) from smallest to largest.
The star at the top of the list is (select all correct answers):
a.
the one that appears dimmest
b.
the one with the smallest luminosity
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c.
the one that appears brightest
d.
the one with the greatest luminosity
Explain your choice(s):
Write the name, vmag, class, and distance for your FIRST FOUR STARS and LAST FOUR STARS
below.
name
vmag
class
distance
First star: ___
HIP 5496
____
____
9.80
____
_____
STAR K0
_____
____
7.474959
____
Second star: _
HIP 51317
______
____
9.65
_____
____
STAR M2
_____
___
7.474959
___
Third star: _
HIP 88574
____
____
9.37
______
_____
STAR M2V
_____
___
7.474959
___
Fourth star: _
HIP 49986
___
____
9.26
_____
______
STAR M3
____
___
7.474959
____
4
th
to last: _
HIP 10625
___
_____
11.96
______
____
STAR M4e
_____
___
7.474959
___
3
rd
to last: _
HIP 76901
___
_____
11.83
_______
____
STAR M5
_____
___
7.474959
___
2
nd
to last: _
HIP 93449
___
_____
11.57
________
____
STAR A5II
______
__
7.474959
____
Last Star: _
HIP 33499__
__
_____
10.81
_____
____
STAR M4
_____
___
7.81311
____
Which star is APPARENTLY the brightest of the 8 stars?
The one with the smallest vmag on the list is the 4th star (HIP 49986), whose vmag is 9.26.
Does this star also have the largest luminosity? ___
no
______ Explain:
When taking a look at the classes for the stars, HIP 49986 is listed as a M3 star, meaning that it’s actually one of the
weakest stars. HIP 93449’s listed as a A5II star, which means that it could be listed higher.
Which star is APPARENTLY the dimmest of the 8 stars?
Star HIP 33499, who’s vmag is 10.81.
Does this star also have the smallest luminosity? ___
no
_____ Explain:
Despite the fact that this star’s class is a M4, it’s actually not the one with the smallest luminosity. Rather, that
would go to HIP 76901, which is classified as Star M5.
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Look at the spectral classes of the stars at the top and bottom of the list. Do you see any correlation?
Yes.
______
If so, describe it:
I noticed that a lot of the stars are actually classed in M, which means that they aren’t really that bright when
compared to others.
Now return to the HIPPARCOS data archive:
http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3table.pl?tablehead=name
%3Dhipparcos&Action=More+Options
This time, instead of selecting for a particular parallax range – which gives you a list of stars that are all
approximately the same distance from you – select for a particular vmag range, which will give you a list of stars
that all APPEAR about the same brightness as seen from Earth. You might need to play with this a bit to get at least
20 stars in your list.
Check the following boxes:
name
parallax
Vmag
bvcolor
class (this is the last row)
At the bottom of the table of possible parameters, you will see the following:
4. Do you want to change your current query settings?
Object Name Or
Coordinates:
(e.g. Cyg X-1 or '12 00 00, 4 12 6') Use semi-
colons (;) to separate multiple object names or coordinate pairs
(e.g. Cyg x-2; 12.235, 15.345)
Coordinate System:
Search Radius:
Default uses the optimum radius for each catalog
searched.
Name Resolver:
Observation Dates:
Not all tables have observation dates. For those
that do, the time portion of the date is optional. Separate
multiple dates/ranges with semicolons (;). Range operator is '..'.
(e.g. 1992-12-31; 48980.5; 1995-01-15 12:00:00; 1997-03-20 ..
2000-10-18)
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Limit Results To:
rows
Output Format:
Show All Parameters:
Select to display all catalog parameters instead of only
defaults
Change “Output Format” to “excel compatible.”
Now select a vmag range. You are welcome to choose any magnitude range, as long as the resulting list has at least
20 stars. The lowest magnitude you can choose is -1.44 (this corresponds to the star Sirius, the brightest star in the
night sky) and the greatest is 14.08. At first try ranges of 1 magnitude, but this might have to be adjusted
depending on your starting magnitude.
Delete any stars for which the Class is “UNIDENTIFIED.”
If your resulting list has more than 20 stars, delete the
rows after the 20
th
star.
Now sort the list according to vmag from smallest to largest.
The star at the top of the list is (select all correct answers):
a.
the one that appears dimmest
b.
the one with the smallest luminosity
c.
the one that appears brightest
d.
the one with the greatest luminosity
Explain your choice(s):
I chose B for this because with the larger positive numbers, this means that the luminosity is actually very dim; the
list represents the stars as it gets brighter. Assuming that the magnitude is the absolute value, the stars located at
the bottom are actually the brightest, not the top.
Compare this list to the one you generated when you selected stars by their parallax. Can you see any obvious
differences between the lists? Be sure to look at all the various values you’ve tabulated, even though you have not
yet been introduced to all of them. An easy way to do this is to “sort” by those values in each list and look at any
trends. Describe any differences between the lists in detail.
Yes, the list is much more filled in comparison to the first list. When looking, I noticed that the set of particular
stars were much closer and similar to each other, than the previous one. There’s no sharp jumps in the rankings, so
I can assume that the stars MIGHT be closer to each other than the ones from the first set would be.
Which list (if either) do you think is
most
representative of the stars in the universe: The parallax-selected list or
the magnitude-selected list?
I think the magnitude-selected list is more representative of the stars in the universe.
Explain your choice:
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I chose this choice because the data for the table seems more completed than the one for the parallax. As we
know, the closer the object is, the dimmer the light is. However, while apparent magnitude is similar (to a degree),
it can be backed up by the absolute magnitude, thus giving us an actual answer for the luminosity.
We will return to these data in later activities.
The exact relationship between apparent magnitude, absolute magnitude, and distance is:
Mv = Vmag – 5logd +5
Where Vmag is the apparent VISUAL magnitude, Mv is the absolute magnitude, and d is the distance to the star in
parsecs.
We are now in a position to find the absolute magnitudes of the stars in the table from the Parallax
Activity. To do this, you will need to open that table, click f(x) and choose SUM. Then enter in the various boxes to
be summed. They are:
5
(the cell number for vmag)
-5*LOG10(cell number for distance)
Cut out your resulting data table and paste it here:
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How many stars in your list have absolute magnitudes LESS than 4.74? In other words, how many stars in your list
are MORE luminous than the Sun?
0.
You know from Unit 2 that the Sun’s spectral type is G2. Does that seem to fit in the absolute magnitude sequence
that you’ve generated? Explain.
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After examining the chart, I can say that the stars in my chart would have to be stars that are lesser than G2. All of
the magnitudes listed are greater than 4.74, which means they are less luminous than the Sun.
ONCE YOU HAVE ANSWERED THE QUESTIONS AND CREATED YOUR DATA TABLES, TURN THIS LAB ACTIVITY IN
VIA BLACKBOARD. Be sure to meet the specific lab deadline.
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