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SMO Overview

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SMO Overview – PowerPoint PPT presentation

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Title: SMO Overview


1
A Journey Through The Universe
2
Lunar Eclipse
3
Eratosthenes Experiment
4
Where Do I work?
UKIRT

Joint Astronomy Centre
JCMT
5
United Kingdom Infrared Telescope
6
James Clerk Maxwell Telescope
7
Most of the Time
8
And Sometimes
9
Topside
10
A View Towards Sagittarius PRC-98-30
11
The Orion Nebula PRC-95-45a
12
Inside Orion PRC-97-13
13
Young Stars With Disks PRC-95-45c
14
Solar System Formation
15
M17 A Wider View PRC-03-13
16
N44F in the LMC PRC-04-26
17
NGC 604 PRC-96-27
18
A Stars Life
19
The Helix Nebula NGC 7293 PRC-03-11
20
The Eskimo Nebula PRC-00-07
21
Supernova
22
Distant Supernovae PRC-98-02
23
The Crab Nebula PRC-00-15c
24
Getting Closer To The Crab PRC-00-15b
25
LMC N49 PRC-03-20
26
A Black Hole In NGC 4261 PRC-92-27
27
A Jet From A Black Hole PRC-99-43e
28
Black Hole In M87 PRC-94-23b
29
Black Hole In M84 PRC-97-12
30
Galaxy Types
31
Hubbles Galaxy Tuning Fork PRC-99-34
32
NGC 4622 PRC-02-03a
33
NGC 3949 PRC-04-25
34
NGC 1300 PRC-05-01
35
Hickson Group 87 PRC-99-31
36
Polar Ring Galaxy NGC 4650A PRC-99-16
37
Looking For A Blank Piece Of Sky PRC-96-01h
38
Hubble Deep Field North PRC-96-01
39
Distant Supernova PRC-01-09
40
Supernova SN2002dd In The HDF PRC-03-12
41
Accelerating Universe PRC-01-09
42
Probing the History of the Universe PRC2004-07
43
A Slice of Time
44
The Fate Of The Universe PRC-9919
45
Composition Of The Universe PRC-01-09
46
Stuff in the Universe
47
Cosmic Tug
48
Cosmic Tug PRC-06-52
49
Crunch, Coast, or Rip?
50
Solar System Formation
51
Ancient astronomers invented geocentric models to
explain planetary motions
  • Like the Sun and Moon, the planets move on the
    celestial sphere with respect to the background
    of stars
  • Most of the time a planet moves eastward in
    direct motion, in the same direction as the Sun
    and the Moon, but from time to time it moves
    westward in retrograde motion

52
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53
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54
A planet undergoes retrograde motion as seen from
Earth when the Earth and the planet pass each
other
55
Johannes Kepler proposed elliptical paths for the
planets about the Sun
  • Using data collected by Tycho Brahe, Kepler
    deduced three laws of planetary motion
  • the orbits are ellipses
  • a planets speed varies as it moves around its
    elliptical orbit
  • the orbital period of a planet is related to the
    size of its orbit

56
Keplers First Law
57
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58
Orbital Shapes
59
Keplers Second Law
60
Keplers Third Law
  • P2 a3
  • P planets sidereal period, in years
  • a planets semimajor axis, in AU

61
Planet Distances Chart
62
Planet Sizes
63
Solar System Sizes
64
Planet Sizes Chart
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