LEFT: The trajectory shows the known visitor from interstellar called 1I/2017 U1
(Oumuamua). 1I stands for 1st Interstellar. Discovered in 2017 by a
military Pan-STARRS 1 telescope in Hawaii at a distance of 0.22 AU from Earth,
the small object came from the direction of the constellation Lyra, cruising through
interstellar space at 26.33 km/s. Its classification as a small comet
vs. asteroid ejected from another planetary system has changed over time:
c,a,c,neither. The second, much larger interstellar object, shown by yellow line,
is 2I/Borisov comet. It's speed in faraway space (32.2 km/s) and the perihelion
distance (2AU) are larger, therefore the deflection angle after flyby is much
smaller than 1I's. Notice that 2I came a short time after 1I.
Click image to enlarge.
CENTER: A visitor from Oort Cloud has been spotted in March 2022 by Californian
astronomers. The Green Comet or C/2022 E3 (ZTF) flew closest to us on
1 Feb 2023, at a safe distance of 0.28 AU. Green light was due to a complex
interaction of UV sunlight with C2 molecules it ejected
(among others).
This comet was initially classified as an asteroid, and may or may not become
interstellar after this passage through the inner Solar System.
RIGHT: A large (up to 9 km radius) Oort cloud comet C/2017 K2 PanSTARRS, passing
by stellar cluster M10 in 2022 near its 1.797 AU perihelion. On nearly-parabolic
inbound orbit (aphelion ~50000 AU), it started outgassing & creating coma early
on (beyond the distance of Saturn), probably due to the CO ice sublimation.
We empahasize theory, but confront the theories with observational facts, including some of the newest discoveries. Part of our course deals with small bodies and dust, an important component of circumstellar dust disks, which represent young planetary systems. At the end, we consider the basic astrobiology.
"Fundamental Planetary Science: Physics, Chemistry and Habitability"
by Jack J. Lissauer and Imke de Pater (2013, 2019). I will mention where
to find the book in the tutorial.
Be careful not to confuse it with the book "Planetary Sciences" (by the
same authors), which is a different, graduate-level, version of the book I mention
in the section on other books.
You don't have to read the whole book. Several chapters might give you
another angle on or another wording of issues than Lectures, but they are not
required reading. Only Chapter 15 is obligatory, please read it.
Grading is standard: minimum percentage marks for letter grades
(for orientation only, since grades are reported as percentages)
A+ 90%, A 85%, A- 80%, B+ 77%, B 73%, B- 70%, C+ 67%, C 63%, C- 60%,
D+ 57%, D 53%, D- 50%, F 49% or less.
*)- the activity points are awarded for participation in lectures and tutorials, and asking questions. Full points will be awarded for coming to office hour and sharing the knowledge gained from reading an optional book, if the level of the book is appropriate, subject concerns planetary systems, and I find that you understood the book. Examples of appropriate books are linked in the previous section. Email me the author and title of a book that is not on the list of recommended books, or show it in person. It will need to be approved (scope, level).
Preferably use mail.utoronto.ca service, avoid sending mail from gmail. UTSC mailer has problems with responding to gmail. Please mention your student number when discussing your personal questions or marks (the temporary results file only lists the last digits of your student number, not your name.) Do not send email or comments to me via Quercus (I rarely check things there, and it's impossible for me to reply.)
Office hours: between lecture and tutorial & immediately after tutorial.
Please remember to number the pages and sign all of them with your name and last 3 digits of student number, say, "...123". Write legibly; very messy homeworks cannot be graded. Please give enough details IN WORDS of the solution procedure. It's as important as the correct final answer. And don't forget to follow the guidelines on what a decent solution must contain (below) such as checking physical units.
Everything you submit and the comments by the marking TA will be visible on Quercus. It will allow multiple submission of the files before deadline, so if you have corrections to your solution please post an updated file before the deadline (so it's not marked as late). You will be able to see and check a computational/calculational solution against a published one. This will make long explanations by the marker (TA) unnecessary, so don't expect very detailed comments on Quercus. Individual problems will have a nominal point value displayed, and the TA will report your marks relative to these max scores. But the eventual "out of" or maximum score for a given task will be decided by the lecturer, and sometimes slightly re-adjusted toward the end of the course in your favor. Check the preliminary results file further down on this web page. The "out of" line gives the number of points yielding 100% mark for a given task.
There are no extensions for assignments.
It is both because of the fairness to all those who respect deadlines, and the
pedagogic needs (right after the deadline we post and/or discuss solutions in
the tutorial.) AccessAbility students will receive an accommodation consisting
of 12-13 days to solve assignment.
Either late submission or point transfer will be done at the discretion of
the professor only in proven medical or personal or family
emergency/bereavement, which you will need to prove in the
University-prescribed way [either Absence (Self-)Declaration via ACORN,
only 1 week allowed per term, or University Verification of Student
Illness/Injury (VOI), which is a doctor's note. Send me the document.]
Likewise, a special treatment will be extended to justified & documented absence at midterm. There are no deferred midterms in ASTC25. Points will be transferred to final exam; you must submit a self-declaration on Acorn and send me a copy, see this page).
Please do not ask for individual extensions because of assignments/exams in other courses - such circumstances are not emergencies, not a sufficient ground for exceptions, and granting them would be unfair to others. Work in other courses should be known and taken by you into account ahead of time. Use the extra 2 days you have to solve any scheduling problems.
If there are misprints or anything else unclear about the problem set and/or
access to it, please ask immediately and allow up to a day for an answer. It
is too late to ask one day before the due date.
Set A1. Due Thu 30 Jan. Formulation
Prob. set 1, PDF . Solutions :
cf. this PDF .
Set A2. Due Thu 13 Feb. Formulation:
In this PDF . Use summary of facts on orbital motion from A1.
Solutions:
cf. this PDF.
Set A3. Due Thu 13 March. Problem formulation:
In this PDF.
Solutions of A3:
this PDF
Set A4. Due Thu 4 Apr 10pm.
Last set:
this PDF.
Solutions:
this PDF
Q: What is the format of the final exam?
A: Exactly the same as midterm, just longer. The level of difficulty is also
the same. 2/3 of final are from the post-midterm material, 1/3 from the
pre-midterm material.
Q: Are exams open-book?
A: No they are not. Electronic devices except calculator are also
prohibited.
Q: Are own notes allowed at exams?
A: YES, own handwritten (not photocopied) notes are allowed: 4 pages
at midterm, 8 pages at the final. That's pages, not sheets. You decide
if the notes are single-sided or double-sided, and what to write in them.
(There is no need to copy tables of planetary data, since all the constants
needed for the solution will be provided in the exam.) You retain the
midterm notes, you can re-use them during the final.
Q: Until when can I drop the course without academic penalty?
A: Until about 25 March or so, google the UTSC sessional dates listing.
Q: Is my presence at *all* lectures and tutorials required?
A: It isn't enforced or mandatory, but it expected & VERY helpful for you to
attend both the lectures and the tutorials. The lectures DO NOT follow
literally a single book or 2 books, except for sometimes quoting the assorted
fragments of our textbook 1 (book no.1 above). Advantages of participating in
meetings are many:
(i) the points for participation (see Marking section),
(ii) you get information beyond what's in the textbook and posted materials,
some of which may be *very* valuable at test/exam. I strongly encourage and
expect you to engage and take own notes (I do write some things on the
blackboard or whiteboard). Not everything will be recorded. Most of the
(exo)planetary system theory is not yet found in any undergraduate
textbooks, so hearing it presented in our meetings will be helpful.
We will be discussing solutions to home assignments and solving new problems
during the tutorials. Tutorials are your ability to use the theory,
in the written part of exams, and beyond.
Q: Will there be recordings of lectures made available and can't I just
use them instead of coming to in-person meetings?
A: We provide lots of material online but it does not replaced lectures or
tutorials.
Recordings from earlier years or from AURA (semi-automatic system)
will be posted in Media Gallery on Quercus. There are occasional glitches in
both, including downtime of microphone because batteries fail, bad visibility
of blackboard, and so on. The course is in-person, so you should not primarily
rely on recordings but attend all the lectures & ask any questions you have
in class or during the break. You will also have the current PDF lecture
notes and some tutorials writeups, below. Re-download them every week, since
a small part of each file is normally updated or expanded shortly before and
sometimes after the lecture.
Q: I have a schedule conflict with another course. Can I skip all the lectures
(or all tutorials)?
A: If you have a scheduling conflict, a fair advice would be: preferably drop
the other course or, if need be, this course.
If you cannot follow this advice, you'll have to rely on recordings, which
are not guaranteed to be full and of high quality, especially of the tutorials,
which are impossible to record well.
Q: Is this page going to be always visible or should I download things I need
from it to my computer?
A: It did happen once that the 'planets' server became unreachable 2 days before
the exam. The networking problem was solved in the last minute, putting a lot of
stress on those who did not download the preperatory material ahead of time. Set
up a directory on your computer and download or refresh lecture notes and other
files you may need (syllabus etc.) need every week, e.g. during the lecture.
There will be two written problems. They require calculations. Use the blank pages of exam booklet as scratch paper. We won't mark those. Your final solution should be legibly written on lined pages.
You do the Quiz on the supplied exam sheet (please do not list quiz answers
in the exam booklet!)
Mark the correctness of the sentence (Y/N) in front of the sentence.
If you answer N, please also circle at least one word or number
which is incorrect, otherwise your answer will be treated as a guess
(no penalty but no credit, either).
Written part requires calculations. If you need scratch paper for that, use
the blank pages of the exam booklet. We won't mark those. Your final solution
must be found legibly written on lined pages.
Everything that was in the lectures and tutorials (and assignments) up to the reading week can be the subject of midterm exam, so study the notes up to and including L10 (up to SPH simulation of star cluster formation), all posted recordings, and the tutorial notes.
Midterm Quiz will be testing notions and facts discussed in Lectures. The texbook may provide additional clarifications but is not required for the midterm. (This may not be the case in the final exam, chapt. 15 of Lissauer/de Pater book will need to be read.)
Own handwritten notes and calculators will be allowed at midterm (see FAQs above). Nothing else is allowed, no electronic devices during the exam. Quiz usually takes about 20 min. You decide what to do first, quiz or written part. But remember that they carry approximately the same weight, so probably doing Quiz first makes more sense.
A training set of quiz questions
is provided below. This version has about 50% of answers provided.
Not sure if the scope exatly covers all lectures up to the SPH simulation
of star cluster formation in L10 (the required material are all
lectures up to this point).
PDF.
Next I provide a set of sample written problems .
Just like the Quiz, to prepare well for the exam, please solve the
unsolved items with or without the lecture notes and texbook in hand.
Problems without solutions .
And here is the set of the problems with most answers or hints provided, but
you should use it after you find your own solutions:
problems-with-solutions .
Remember that a fully solved problem (in exam or assignment) may require all 6 points listed earlier in the section on homeworks.
Study the format of midterm in this actual 2024 midterm file.
midterm 2024 w/solutions. There may be some overlap with the preparation
files above.
In 2024, the midterm problem was about:
As to the written problems, please also remember to check the preparatory material for the midterm and all the posted homeworks & their solutions. I'm not including those things in the problems below, although I have covered most of the course material in preparation file for the Quiz.
The problems WITHOUT solutions, PDF file . The problems WITH solutions, PDF file .