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Discovery of Uranus, Neptune, Pluto

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Title: Discovery of Uranus, Neptune, Pluto


1
Discovery of Uranus, Neptune, Pluto
  • The last 3 planets were discovered with
    telescopes, in the last 150 years or so (too
    faint to see with eyes)
  • Studied (glimpsed) by Voyager 2, powered by
    gravity slingshot explored all Jovian planets
  • Uranus was discovered accidentally by William
    Herschel
  • Neptune was discovered mathematically!
    Following observations of perturbations in the
    orbit of Uranus by an unseen object, Adams and
    Levellier independently predicted its existence
  • Pluto is not a (Jovian) planet, more like a
    moon, planetesimal, or asteroid was discovered
    in 1930 by Clyde Tombaugh

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Uranus
4
View of Uranus from Earth(something strange ?)
5
Orbit of Uranus around the Sun Rotation axis
tilted at 98 degrees !
6
Uranus
  • Uranus and Neptune are almost twins in size
    25,000 Kms radius
  • Uranus is tilted on its side by 98 degrees each
    pole faces the sun for half the orbital period
    (84 years)
  • Cause of tilt? Where on Uranus would you go to
    spend summer vacation ?
  • Uranus rotates somewhat backwards like Venus
    rotation period 17hr 14m
  • Weak magnetic field 0.74 x Earths, could be a
    very small metallic mantle
  • Methane atmosphere, hence greenish hue
  • H2O (ice) mantle

7
Neptune
8
Neptune and the Great Black Spot
9
Methane ice clouds on Neptune
10
Atmosphere of Neptune (c.f. Jupiter)
A pale imitation of Jupiter!
11
Neptune
  • Neptunes atmosphere very active, with
    convection currents
  • Great Black Spot 10,000 Kms long, cyclonic
    storm like the GRS on Jupiter
  • Internal energy source (gravity) like Jupiter
    emits 2.6 times the energy it receives from the
    sun
  • Tilted at 30 degrees
  • Strange moon Triton, which rotates backwards,
    probably a captured Kuiper Belt Object
  • Magnetic field tilted 50 degrees to rotation
    axis mag poles not aligned with geo poles (Earth
    and Jupiter are about 10 degrees)

12
Magnetic and geographical axes
Neptunes Magnetic axis is NOT centered
13
Structures of Uranus and Neptune
Relatively thin atmospheres compared to Jupiter
and Saturn, but still quite extensive compared
to terrestrial planets
14
Atmospheres of Uranus and Neptune
  • More He than Jupiter and Saturn
  • Insufficient gravity ? loss of H
  • H is locked up in methane CH4, 10 x Jovian,
    (also more carbon) ? absorbs red, reflects blue
  • Hydrocarbon smog mainly frozen methane haze
    and clouds with ethane, acetylene, etc.
  • Discovery of Jupiters ring(s) by Voyager 2

15
Discovery of Ring Systems in Jovian Planets
  • Jupiter --------- Voyager 2
  • Saturn --------- Galileo
  • Uranus --------- Occultation
  • Neptune --------- Occultation
  • - Occultation ? Obscuration of starlight by
    rings
  • - Jupiters ring is very thin and dusty material

16
Occultation of starlight by rings of Uranus
Dusty rings of Uranus not seen from the Earth
occultation method used following the discovery
of Jupiters ring by Voyager 2
17
Occultation Spectrum due to rings of Uranus
dimming of starlight blocked by the rings as seen
from the Earth
18
Uranus rings and moons
19
Uraniun system with rings
Note the rotation axis and position of rings
20
Voyager 2 view of Rings of Uranus(dusty,
extended atmosphere makes rings unstable)
Relatively more extended atmospheres due to lower
gravity than Jupiter and Saturn
21
Neptunes rings (similar to Uranus dusty
ambient atmosphere)
The slit in the middle blocks out light from the
main body of the planet, Thereby enabling the
faint rings to be seen
22
Rings of Uranus and Neptune
  • Both Uranus and Neptune have ring systems
  • Made mainly of rocks, not ice like Saturn,
    therefore nearly invisible
  • Owing to low gravity, the ring structures are
    diffuse and unstable extend into the moons
    (hence heavily cratered) or spiral into the
    planet
  • Probably last no more than 10-100 million years

23
Moons of Uranus and Neptune
  • Uranus has 5 large moons, and 10 small ones, all
    heavily cratered
  • Miranda shows large oval structures may have
    shattered several times and re-assembled
  • Neptune has 5 small moons (lt 100 Kms) bunched
    near the rings followed by Proteus at 200 Kms,
    and then Triton
  • Uranus and Neptune do not have large Galilean
    satellites did not form moons on their own as in
    Jupiter and Saturn

24
Moons of Uranus heavily cratered due to
interaction with loose ring particles and dust
25
Miranda Broken and re-assembled ?
26
Triton captured by Neptune ?
Orbits opposite to direction of rotation of
Neptune
27
Triton
  • Triton is more dense, 2 g/cc, indicating rocky
    composition, than the moons nearer to Neptune
    which are mostly ice
  • Reverse of the trend for Galilean satellites
  • Triton might have been a Kuiper Belt Object,
    captured by Neptune
  • Has a very thin atmosphere, 0.00002 bars
  • T 38 K ? N and CH4 freeze and snow
  • Polar caps extend to 25 degree latitude

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