astronomy 105 laboratory lab 08 · 2018-07-02 · 300 ly heliocentric parallax 1 a.u. 1 au radar...
TRANSCRIPT
LAB 08
Astronomy 105 Laboratory
STELLAR PARALLAX
Lab 08 – Part 1
Heliocentric Parallax300 ly
1 AU Radar1 A.U.
Main-Sequence Fitting30,000 ly
Variable Stars300 Mly
billions of ly WD Supernovae
Cosmic
Distance
Ladder
Stellar Parallax
Sky - Angular Measurements
Locate “Star A” above the reference stars and “Star B” below
X
Distant
background
starsX
X X
Angular shifts
Telescope Field of View and Scale
Image of star Field
?
28”
A B
Known separation of stars A & B is 28 arc seconds
What is the angular separation of Stars C & D?
Find a unit conversion ( cm to arc seconds).
Measure the distance between A and B.
28 arc seconds is equivalent to 0.8 cm.
28 arc sec = 0.8 cm
0.8 cm
0.8 cm28 arc sec=
0.8 cm
cm1
arc sec=35
Plate Scale
Angular separation of Stars C & D
2.5 cm X 35 cm
arc sec = 88 arc sec
CD
MAIN-SEQUENCE FITTING
Lab 08 – Part 2
Open or Galactic Cluster
M13 - Globular Cluster
Distance-23,000 ly Size-150 ly
Finding a Star’s Distance
Stellar Parallax
Main-Sequence Fitting
1 2 3 4 5 6Brighter Dimmer
Magnitude Scale
Brightest stars in the night sky Faintest stars visible to
naked-eye
Measuring a Star’s Brightness
2.512
Magnitude Difference
Brightness Ratio (Brightness Difference)
1 (2.512)1 2.5 2 (2.512)2 6.3 3 (2.512)3 15.9 4 (2.512)4 40 5 (2.512)5 100 6 (2.512)6 251
Magnitude
Stellar Brightness
Apparent Magnitude (mv) - Brightness from Earth
Absolute Magnitude (Mv) - Brightness from 10 pc
Photometer
(measures
brightness)
10 meters1/4
Apparent Brightness and the Inverse-Square Law of Light
Apparent Brightness 1/d2
If this 100 Watt light bulb were observed to be 100 times fainter compared to the 10 meter distance; how far away is it?
√100 = 10
10 times farther away or 10 x (10 meters) = 100 m
100 W
100 W
100 W
100 W
20 meters
30 meters
40 meters
1/9
1/16
1370 watts/m2 343 watts/m2 55 watts/m2
Apparent Brightness 1/d2
Apparent Brightness and the Inverse-Square Law of Light
1 AU
= 4____1370
343
4 = 2
2 AU
= 25____1370
55
25 = 5
5 AU
Mv = 5
mv = 10
10 pc
Is the star closer than 10 pc
or farther away than 10 pc?
?
How much farther?
Distance Modulus = m - M
Distance Modulus = 10 – 5
If m-M > 0 then star’s distance > 10 pc.
If m-M = 0 then star’s distance = 10 pc.
If m-M < 0 then star’s distance < 10 pc.
Brightness Difference = 2.5125 = 100
= +5
Inverse-Square Law - Apparent Brightness ~ 1/d2
Star is 10x farther away than 10 pc or 10 X 10 pc = 100 pc
G2 V
√100 = 10
Finding a Star’s Distance
1. Brightness at standard distance (10 pc)
• Absolute magnitude
2. Measure apparent brightness
• Apparent magnitude
3. Use inverse-square law of light to find distance
Hyades Star Cluster
Pleiades Star Cluster
Taurus
Main-Sequence Fitting
Stars in a Cluster•Common Properties
•Distance
•Age
•Different Properties
•Spectral Types (temperature)
•Luminosity Class (size)
Main-Sequence Fitting
Pleiades stars have the same luminosities as the Hyades stars.
The Pleiades is 2.73 times farther away!
√7.5 = 2.73
They are farther away!
How much farther?
Why are the Pleiades stars 7.5 times dimmer?
Interstellar Dust
Reddens Light (stars appear cooler)
Dims Light (stars appear further away)
-4
-3
-2
-1
0
1
2
3
4
5
6
7
8
9
10
11
12
-0.4 -0.2 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4
Ab
so
lute
Ma
gn
itu
de
(M
v)
Color Index(mb-mv)
Standard Main-Sequence
Pleiades Color-Magnitude Diagram
3.0
4.0
5.0
6.0
7.0
8.0
9.0
10.0
11.0
12.0
-0.30 -0.20 -0.10 0.00 0.10 0.20 0.30 0.40 0.50 0.60
Color Index
(mb-mv)
Ap
pa
ren
t M
ag
nit
ud
e (
mv)
9
1820
31
27
22
Color Index = 0.415
mv = 9.8temperature
Standard Main-Sequence
-3.0
-2.0
-1.0
0.0
1.0
2.0
3.0
4.0
5.0
6.0
-0.30 -0.20 -0.10 0.00 0.10 0.20 0.30 0.40 0.50 0.60
Color Index
(mb-mv)
Ab
so
lute
Ma
gn
itu
de
(M
v)
Color Index = 0.415
Mv = 3.6
mv = 9.8
mv – Mv = 9.8 - 3.6 = +6.2
1. Using the average distance modulus
from several stars, calculate the
distance to the Pleiades star cluster.
2. Use the main-sequence fitting
technique to find the distance modulus
and calculate the distance to the
Pleiades again.
-4
-3
-2
-1
0
1
2
3
4
5
6
7
8
9
10
11
12
-0.4 -0.2 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4
Ab
so
lute
Ma
gn
itu
de
(M
v)
Color Index(mb-mv)
Standard Main-Sequence
-4
-3
-2
-1
0
1
2
3
4
5
6
7
8
9
10
11
12
-0.4 -0.2 0.0 0.2 0.4 0.6 0.8 1.0 1.2
Ap
pa
ren
t M
ag
nit
ud
e (
mv)
Color Index(mb-mv)
Pleiades Color-Magnitude DiagramAbsolute
Zero
Magnitude
THE END