Click on the image of a transiting planet (HD209458b, 3.5 day period
"hot Jupiter") to view the graph of 110+ extrasolar planets
(distances, masses). See the whole site of Geoff Marcy's group of
planet
hunters in Berkeley . They have
found most planets to date, but the European team of Michel Mayor in
Geneva follows closely (in 1995 they've found the first exoplanet
around a solar-type star, 51 Peg b).
UNDERGRADUATE COURSE INFORMATION
Title:
Planetary Systems (AI 1400)
Term: Fall 2004
Teacher: doc Pawel Artymowicz (tel 08
5537-8549; pawel@astro.su.se)
Teaching Assistant: Magnus Galfalk (tel.
-8553; magnusg@astro.su.se)
Times of lectures : 10:15 am - 12:00 am
(with a short break)
Place: Stockholm Observatory SCFAB (Albanova
Ctr), 6th floor, seminar room C6:61
Dates of lectures:
October: 19 (Tue), 21 (Thu), 26 (Tue), 28(Thu)
November: 2(Tue), 4(Thu), 9 (Tue),
16*(Tue), 18(Thu), 23 (Tue), 25* (Thu), 30(Thu)
December: 7 (Tue) = Exam
2 problem sessions: 13:15 - 15:15;
their dates are denoted by * above
Dates/times of 2 laboratory excercises:
to be arranged with the TA (teaching asst.)
Date of the final exam: 7 December
(Tuesday), 10.00-12.30 and 13.15-14:45
Omtentamen (re-exam) about 10 days later.
Basic course reference: J. Kelly Beatty, C.
Collins Petersen, A. Chaikin (Eds.), "The New Solar System" 4th Edition
(important!) (Cambridge Univ. Press, 1999)
Notice, however, that at present, no appropriate textbook covering the
whole course exists, so you will rely
on your own notes from the
lectures (including those things you decide to xerox from my
viewgraphs), and some materials placed on these web pages in electronic
form
(scanned viewgraphs and pictures).
Many students have in the past asked me for precise guidance on
which parts of this book to read. OK, please do pay attention to
these chapters:
1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20,
21, 22, 23, 24, 25, 26. (no, just kidding!) Here it goes: * means
especially recommended for the test.
2*, 5*, 6, 12*, 13, 14*, 15, 16*, 23, 24, 25, 27, 28*.
About a week before the exam I'll provide warm-up test questions of the
type
later asked (YES/NO questions).
Suggested additional reading includes:
o Internet
(we recommend www.google.com
to look for keywords; as well as the links below);
o Stuart Ross
Taylor, "Solar System Evolution", 2nd Edition, Cambridge U. Press, 2001
;
o Imke de
Pater, Jack J. Lissauer "Planetary Sciences", Cambridge U. Press, 2001;
o David
Morrison, Tobias Owen "The Planetary System", 3rd Edition, Addison
Wesley, 2003;
o J. Benett,
S. Shostak, B. Jakosky "Life in the Universe", Addison Wesley, 2003;
Course grading will be based on:
4 sets of homework problems posted on this
page (20% of the total score),
the written exam (45% for problems, 35% for test = a
large set of Yes/No questions).
>75% of the max score required for VG, >50% for G
grade.
Lab exercises are required to be successfully done and
described to TA's satisfaction.
SYLLABUS (TOPICS)
with some links to electronic materials
Note: topic numbers do not, in general,
coincide
with lecture number.
- Gentle introduction to planetary systems
- Gravitational mechanics of planetary systems
- Formation od planetary systems
- Minor bodies of the Solar System
- Interplanetary dust: zodiacal light
- Interplanetary dust: zodiacal light
- Interplanetary debris: Meteoroids and meteorites
- Asteroids
- Comets
- Planetary interiors
- Rotational flattening
- Terrestrial planets and moons
- Giant planets
- Extrasolar planets: gas giants or rocky balls?
- Surfaces of Solar System bodies
- Impact cratering
- Volcanism and tectonics
- Erosion
- Atmospheres
- Hydrostatic equilibrium and escape of
atmospheres
- Terrestrial atmospheres
- Giant planet atmospheres
- Planetary rings
- Discovery of rings
- Resonances and waves in disks, ring
shepherding
- Ring galore
- Extrasolar planetary systems
- Search techniques
- Pulsar planets
- Vega-type systems: footprints in the dust and
sand
- Beta Pictoris disk: evidence of planetesimals
and planets
- Replenished dust disks: nature or nurture?
- Transitional disks and the dust-gas
interaction
- Radial velocity systems I: Clues to their
origin
- Radial velocity systems II: What do they
teach
us about our system
- Astrobiology
- Drake's equation
- Habitable zones
- Life on Earth
- Life elswhere?
- SETI and the Fermi paradox
Problem set No. 1
Problem set No. 2
Problem set No. 3
Problem set No. 4
SAMPLE EXAM
Here you can see the text files with the final exam of the 2004 course (no
solutions!):
part I (Problems)
and the
part II (Test)
.
About the homework problems
See a guide to the style of solutions of homework
(also the exam) involving math here.
Please remember also to: staple together your
homework or at least number the pages clearly and sign them with your
name. Write legibly: unusually messy homeworks will be returned
to
you. The usually-messy homeworks will be accepted but run the risk of
being misunderstrood and/or underappreciated. Please give enough
details
of the solution procedure. It's as important as the correct final
answer.
Importantly, please keep a copy of your
solutions for yourself (you can use the Observatory copy machine
for
that). Many solutions will be discussed during the problem sessions.
Finally, plan for a timely submission of solutions. Occasional
delays will be tolerated, but very late submissions will earn little
credit.
Useful or just interesting links:
- Multimedia
tour of the nine planets in our system
- Solar
Views = more multimedia including some movies
- The Extrasolar Planets
Encyclopaedia
- EU Research and
Training Network (Stockholm Observatory is one of the nodes, cf below)
- Theory
of Planetary Systems group page at our Observatory
- Giant
Planets Orbiting Faraway Stars - an article by Geof Marcy and paul
Butler
- Exploring
New Worlds - an article by Ron Cowen
- The Swiss
site
about exoplanets
- A fantastic
article-search astronomical database from Harvard
- Maps of our Solar System
bodies
- Solar System Orery
- New STScI press
releases
- STScI Digital Sky
Survey search form. Input ANY object's designation to get coordinates
and .GIF picture
-
Migration Type III. a talk by Pawel Artymowicz at:
-
KITP/UCSB 2004 conference on Planet Formation (abstracts,
streaming audio & video)
The URL of this page is
http://planets.utsc.utoronto.ca/~pawel/planetsys.html
This way to the home page of the
Planet Formation group at the Stockholm Observ. at
http://planets.utsc.utoronto.ca/~pawel/systems.html
This way to the home page of Pawel Artymowicz.