AST221_2023F_Assignment1
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School
University of Toronto *
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Course
221
Subject
Astronomy
Date
Jan 9, 2024
Type
Pages
2
Uploaded by EarlPigeon2903
Assignment 1
AST221H
Due: Sept. 29, 2023
You may work together with other students to solve these problem sets, but all solutions must
be written and submitted independently.
Show your work clearly for full marks, including
intermediate steps, and diagrams if necessary! Answers that are not fully explained will not
get full marks. Check the syllabus for reading recommendations. Include units!
Submit your assignment as a single .pdf file following the instructions on Quercus.
This
includes the plot in Question 4!
Problem 1: Parallax
a (3 points) If parallax can be measured with an accuracy of 0.01 arcseconds, and the
mean density of stars in the Solar neighbourhood is 0.1 pc
−
3
, how many stars can have
their distances measured via parallax? Clearly state any assumptions you make to solve
this problem.
b (2 points) Parallax doesn’t have to be measured using the orbit of Earth as a baseline.
In 1672, an international effort was made to measure the parallax angle of Mars at
opposition, when it was on the opposite side of the Earth from the Sun, and thus
closest to Earth, using two widely-separated observers on Earth.
Consider two observers at the same longitude but one at latitude of 45 degrees North
and the other at 45 degrees South. Work out the physical separation
s
between the
observers given the radius of Earth is
R
E
≈
6400 km.
c (2 points) If the parallax angle measured was 25 arcseconds, using your previous result,
what was the distance to Mars? Give your answer in both km and au (astronomical
units).
d (3 points) If we want to measure the distance to Mars with a precision of 10%, how
closely must the clocks used by the two observers be synchronized? Ignore the rota-
tion of the Earth, and assume the average orbital velocities of Earth and Mars are
29.79 km s
−
1
and 24.13 km s
−
1
, respectively. Explain your answer.
Problem 2: The Alpha Centauri system
a (3 points) The low-mass star, Proxima Centauri, is the closest known star to the Sun,
and has a parallax of 0.77
′′
and an apparent magnitude
m
= 11
.
05. What is Proxima
Centauri’s distance in light years? How much brighter or fainter in luminosity is the
star Proxima Centauri compared to the Sun?
b (2 points) Given your result in a), how close to Proxima Centauri would a planet need
to orbit to receive the same amount of flux as the Earth does from the Sun?
What
would the period be for such a planet?
1
Assignment 1
AST221H
Due: Sept. 29, 2023
c (2 points) In the above, you calculated the luminosity of Proxima Centauri based on
its visual magnitude. Proxima Centauri is a red dwarf star, and is cooler than the Sun.
As we will learn more later, this means that it emits more light at longer wavelengths.
The total, or bolometric luminosity of Proxima Centauri is actually
L
bol
= 0
.
0017 times
the luminosity of the Sun. Given this value, at what distance would a planet orbit to
obtain the same amount of flux as the Earth does from the Sun?
d (2 points) In 2016, it was discovered that there was an Earth-sized planet orbiting
Proxima Centauri at a distance of approximately 0.05 au.
Given your calculation
above, do you think this Earth-sized planet could be Earth-like? Give your reasoning,
including what properties of the planet you are considering when you are judging its
‘Earth-like’ characteristics.
e (2 points) Proxima Centauri is the faintest member of a triple star system. The other
two stars, Alpha Centauri A and Alpha Centauri B, have apparent magnitudes
m
= 0
.
01
and
m
= 1
.
33, respectively. To the naked eye, however, they cannot be resolved into
two separate stars. If you had a telescope with the same resolution as your eyes, what
would the apparent magnitude of this unresolved binary star be?
Problem 3: Jumping into space
(6 points) On Earth, you can probably jump 0.3 m off the ground. On a sufficiently small
asteroid, the same jump would enable you to escape the asteroid’s gravity forever.
If we
assume that this asteroid is spherical and has a density
ρ
≃
2500 kg m
−
3
, what is the
maximum radius such an asteroid can have? Show your work and reasoning clearly.
Problem 4: The mass of Jupiter
(6 points) For this question, refer to the Jupyter notebook on the A1 Quercus page.
Go
through the notebook, and submit your final plot of Jupiter’s moons orbital radii and periods.
Based on your fit results, calculate the mass of Jupiter and show your work.
You will be
better able to complete this notebook after completing the python tutorial notebook from
class on Friday, Sept. 15. For your assignment, please submit separately the .pdf and the
.ipynb files of your
solved
Jupyter notebook so we can check your coding, but include your
plot and calculations in your main assignment submission.
2
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