Transcript Slide set 5

NATS 1311 From the Cosmos to Earth
Jovian planets compared to earth
NATS 1311 From the Cosmos to Earth
NATS 1311 From the Cosmos to Earth
Jupiter and Io
From 29 million miles
away.
Zones- bright cloud
regions, rising/ cooler
gases.
Belts- dark cloud
regions, descending /
warmer gases.
Heating from interior
causes cloud motions.
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Jupiter
Great red
spotGiant
hurricane
twice the
size of earth.
False color
image to
enhance
cloud
turbulence.
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Jupiter’s ring
(artist’s
sketch)
35,000 miles
above cloud
tops.
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Jupiter’s ring
(Actual photo)
4000 miles,
edge to edge.
1 mile thick.
NATS 1311 From the Cosmos to Earth FIG.9.4
Figure 9.4 These diagrams compare the interior structures of
the Jovian planets (shown approximately to scale). All four
planets have cores equal to about 10 Earth masses or rock,
metal, and hydrogen compounds, and they differ primarily in
the hydrogen/helium layers that surround the cores.
NATS 1311 From the Cosmos to Earth FIG. 9.2
Figure 9.2 Jupiter's interior structure, labeled with the pressure, temperature,
and density at various depths. Earth's interior structure is shown to scale for
comparison. Note that Jupiter's core is only slightly larger than Earth but is
about 10 times more massive.
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SCIENTIFIC HIGHLIGHTS - JUPITER
ATMOSPHERE:
CLOUD BANDS - ALTERNATE COLORS
CLOUD MOTIONS BELTS - REDDISH BROWN BANDS - COOLR
ZONES - WHITE, YEEEOW BANDS - HOTTER
COMPOSITION - WATER AND AMMONIA CLOUDS
LIGHTNING AND AURORA OBSERVED
GREAT RED SPOT:
HURRICANE STORM OVER 300 YEARS OLD
TWICE THE DIAMETER OF EARTH
RING:
1 KM THICK, 6000 KM EXTENDED RADIALLY
NATS 1311 From the Cosmos to Earth FIG.9.9
Figure 9.9
The larger
satellites of
the Jovian
planets, with
sizes (but not
distances)
shown to
scale.
Mercury, the
Moon, and
Pluto are
included for
comparison.
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GALILEAN MOONS
Io:





8 volcanoes
Smooth young surface
Sulfur and SO2 frost
Volcanoes eject sulfur material producing a ring
of sulfur and O2 around Jupiter
Magnetic field of Jupiter allows particles to
penetrate the polar regions, producing aurora
NATS 1311 From the Cosmos to Earth FIG. 9.11
Figure 9.11 Io is the most
volcanically active body in
the solar system. (a) An
erupting volcanic plume
rising hundreds of kilometers
above Io's surface. (b) The
reddish color of the nowcooled lava flows extending
from this volcano on Io
(center black dot) suggests
they were once molten
sulfur. (c) This enhancedcolor photo shows fallout
(dark patch) from a volcanic
plume on Io. The fallout
region covers an area the
size of Arizona. (The orange
ring is the fallout from
another volcano.)
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Io
Close-up of surface.
Tidal heating causes
melting under surface
to produce volcanoes.
NATS 1311 From the Cosmos to Earth FIG. 9.12
Figure 9.12 Tidal heating explained. (a) Because Io's orbit is slightly
elliptical, the strength and direction of Io's tidal bulges change. The
bulges and orbital eccentricity are exaggerated. (b) About every
seven Earth days (one Ganymede orbit, two Europa orbits, and four
Io orbits), the three moons line up as shown. The small gravitational
tugs repeat and make all three orbits slightly elliptical.
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GALILEAN MOONS
EUROPA:
Thin ice crust
Fracture/ridge system
Few craters
NATS 1311 From the Cosmos to Earth FIG. 9.14
Figure 9.14 Europa is one of the most intriguing moons in the solar system. (a)
Europa's icy crust is criss-crossed with cracks. (b) Some regions show jumbled
crust with icebergs, apparently frozen in slush. This figure combines lowresolution images and high-resolution close-ups from the Galileo spacecraft. (c)
Close-up photos show that many surface cracks have a double-ridged pattern.
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GALILEAN MOONS
GANYEMEDE:




Bright, young ray craters
Impact basin
Dark regions are heavily cratered
Variety of geologic processes observed
(e.g. crustal motion)
 Largest of the moons
NATS 1311 From the Cosmos to Earth FIG. 9.15
Figure 9.15
Ganymede, the
largest moon in the
solar system. (a)
Ganymede's
numerous craters
(bright spots) show
that its surface is
older than Europa's
(b) The brighter,
ridged regions of
Ganymede's
surface, called
grooved terrain,
have few craters
and indicate
relatively recent
geological activity.
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GALILEAN MOONS
CALLISTO:
Ancient heavily cratered surface
Impact basins
Density low
Little crustal motion
NATS 1311 From the Cosmos to Earth FIG. 9.16
Figure 9.16 Callisto shows no evidence of volcanic or tectonic
activity. (a) Heavy cratering indicates an ancient surface. (b)
Close-up photos show a dark powder overlying the low areas
of the surface.
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Callisto
Large impact basin.
Rings are shock waves that froze quickly after impact.
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Saturn- Ring structure
Tilt of rings 27 degrees from orbital plane.
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Saturn
CloudsBelts and zones
not as pronounced
as on Jupiter
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Saturn ring structure- false color image
Cassini division- large gap in rings
NATS 1311 From the Cosmos to Earth FIG. 9.22
Figure 9.22 (a) The largest gap in Saturn's rings, called the
Cassini division, is caused by an orbital resonance with the
moon Mimas. (b) Another Mimas resonance creates
remarkable ripples in Saturn's rings. The dark spots in the
image are calibration marks for the camera.
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Spokes in B ring
Spokes do not follow
Kepler’s Laws
Magnetic and electric
fields form these
patterns.
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Another view of rings
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Titan, moon
of Saturn
3200 miles diameter
Atmosphere denser
than earth’s.
Nitrogen with some
Methane.
Temperature on
surface: -180 deg. C.
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Comparison of earth and Titan atmospheres
NATS 1311 From the Cosmos to Earth Fig. 9.17
Figure 9.17 Saturn's
moon Titan. (a) Titan is
enshrouded by a hazy,
cloudy atmosphere. (b)
Artist's conception of the
surface of Titan,
showing the possible
ethane oceans. (c) A
recent image from the
Keck Telescope taken at
infrared wavelengths
can see through Titan's
clouds to the surface.
The dark areas may be
oceans.
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SCIENTIFIC HIGHLIGHTS - SATURN
SATURN:
 Atmosphere similar to Jupiter
 Dark belts and light zones
 High winds - 4 to 5 times faster than Jupiter’s
 Cold temperatures (90 k)
 Aurora
 Radio emissions
RINGS:
 Hundreds of ringlets
 F ring - 3 separate intertwined ringlets: also clumps
 B ring has long radial spoke-like features
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SATURN’S SATELLITES:
 23 (9 major moons)
 Number 13 and 14 guard the f ring
 Number 15 is on the outer edge of the a-ring
 Titan:
• Smaller than Ganymede, larger than Mercury
• Has a dense, hazy atmosphere of nitrogen
(methane) and carbon dioxide with
small concentrations of hydrocarbons
• Surface temperature is 100 k (-170°c)
• Liquid nitrogen or methane lakes may exist at
the poles
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NATS 1311 From the Cosmos to Earth
True (left) and false colors images of Uranus
Picture of south pole from 9 million miles away.
South pole, pointed toward sun.
Methane in atmosphere absorbs red light; hence blue color.
Discovered in 1781 by Wm. Herschel.
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Artist’s sketch of Uranus’ ringsdiscovered be stellar occultation.
Rings closer to planet than moons.
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Ring structure
Of Uranus.
Shows dust in
ring system.
Streaks are
stars.
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Miranda,
Moon of Uranus
Cosmic museum
Many unique
features.
“7”
Trapezoidal
region.
Grooved terrain.
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Miranda
Mountainous region.
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SCIENTIFIC HIGHLIGHTS - URANUS
Discovered by William Herschel in 1781
 4 times earth's diameter
 First planet not known to Greek astronomers
 Blue-greenish appearance,with rocky core
 Thick hydrogen atmosphere with methane clouds
 Methane absorbes red light
 Rotation period 16.5 hours
NATS 1311 From the Cosmos to Earth
URANUS (continued)
 Spin axis tipped at 82° to the orbital plane
 Has a retrograde rotation
 Has a 21 year winter and a 21 year summer
 Poles have the same temperature
 Magnetic field is 50 times the earth's tipped 60 degrees
NATS 1311 From the Cosmos to Earth
URANUS (continued)
RINGS:
 10 rings
9 discovered by stellar occultation
1 discovered by Voyager spacecraft
 Probably composed of rocks rather than ice
 Source may have been a moon destroyed by a meteoroid
impact
NATS 1311 From the Cosmos to Earth
URANUS (continued)
MOONS:
 5 largest seen from earth; made of rocks and ice
 10 discovered by voyager spacecraft
 Miranda—many unique surface features,
Chevron, grooved terrain, large valley, high cliffs
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Neptune
Methane absorbs
red light, gives
blue-green color.
Great dark spot,
like Jupiter’s red
spot.
Cloud structure
has belts and
zones, like
Jupiter.
NATS 1311 From the Cosmos to Earth
Neptune’s great
dark spot. About
size of earth.
Same relative
size to planet as
Jupiter’s spot is
to Jupiter.
Atmosphere is
very cold: -350°F
Scooter- cloud
formation below
the dark spot.
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Neptune’s rings
50,000 Km above
planet.
Clumpy, not
continuous.
Probably methane
ice.
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Triton, moon of Neptune. Probably a captured asteroid.
Polar cap, frozen nitrogen.
Wrinkled surface, like Mercury
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Close-up of
Triton’s surface .
70% rock;
30% water ice.
Very old craters.
Circular region
may be volcano
caldera.
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Triton’s surface. The flat regions in this close-up photo may
be lava-filled impact basins similar to the lunar maria.
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SCIENTIFIC HIGHLIGHTS - NEPTUNE
 Discovered in 1845 using mathematical analysis of
Uranus' orbit
 Similar in size to Uranus, but slightly more dense
 Seeing Neptune is like seeing a dime a mile away
 Has a blue-green appearance (methane in atmosphere)
 Internal heating like Jupiter
 Great dark spot, not permanent
 Cloud features seen in atmosphere
 Cloud shadows indicate lower atmosphere is clear
NATS 1311 From the Cosmos to Earth
SCIENTIFIC HIGHLIGHTS - NEPTUNE
RINGS:
Has a system of thin dark clumpy rings
Two thin and two broad rings
 50,000 and 60,000 km above planet
Probably methane ice
8 MOONS:
2 found from earth
6 discovered by voyager spacecraft
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NEPTUNE’S MOONS
 Triton Largest moon of Neptune:
Orbits Neptune in retrograde direction probably a captured asteroid
Slightly smaller than our moon
Has a few craters in the southern region
Has nitrogen frost at poles
Atmosphere of nitrogen with traces of methane
(much less dense than earth's)
NATS 1311 From the Cosmos to Earth FIG. 9.23
Figure 9.23 Four ring systems. The planets are not shown
to scale. Uranus's rings were photographed by the Hubble
Space Telescope, the others by Voyager. The Neptune
frame is made of two images, taken on either side of the
bright planet.
NATS 1311 From the Cosmos to Earth .
NATS 1311 From the Cosmos to Earth .
NATS 1311 From the Cosmos to Earth .
The orientation of Pluto's spin axis and Charon's orbit.
Like Venus and Uranus, Pluto has its rotation axis tipped over so far
that it points below the plane of the planet's orbit (which is itself tipped
by an unusually large angle, 17°, relative to the ecliptic). Thus the
spin of the planet is technically retrograde (i.e., backwards). Charon
orbits in the equatorial plane of the planet.
During the late 1980s, the plane of Charon's orbit was aligned with
thePluto-Earth direction so that Pluto and Charon alternately passed
in front of each other.
Observations of these repeated transit events provided a wealth of
information on the nature of both bodies and the transient
atmosphere of Pluto.
NATS 1311 From the Cosmos to Earth .
SCIENTIFIC HIGHLIGHTS - PLUTO
 Discovered in 1930 by Clyde Tombaugh at Lowell
Observatory
 Not a planet that perturbs Uranus' orbit - too small
 Orbit has a 17º inclination to the ecliptic
 Elliptical orbit which passes inside the orbit of
Neptune (November 1978 to may 2000)
 Rocky core with methane and water ices, also nitrogen ice
on surface
NATS 1311 From the Cosmos to Earth .
SCIENTIFIC HIGHLIGHTS - PLUTO
 Tenuous atmosphere of nitrogen and methane
 May be an escaped moon of Neptune or may be one of
group of icy/rocky bodies in the outer solar system.
Some orbit the Jovian planets and one, Pluto, orbits
the sun
Moon:
 Charon—1978 discovery
Synchronous rotation with Pluto
Only 20,000 km from Pluto
Half the size of Pluto
10% mass of Pluto
NATS 1311 From the Cosmos to Earth .
PROPERTIES OF THE SUN
Diameter:
864,000 miles
Volume:
1 million times that of the earth
Mass:
330,000 times mass of earth
Composition:
Hydrogen
Helium
Other
By mass
75%
24%
1%
By volume
90%
9%
1%
NATS 1311 From the Cosmos to Earth .
SUN
Surface temperature:
Color:
5700 k (5400º C)
yellow
Rotation period:
25 days at the equator
33 days near poles
Apparent magnitude:
- 26.7
Absolute magnitude:
+ 4.8
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LUMINOSITIES
Luminosity:
~ r2T4
Apparent magnitude:
Apparent brightness of a
celestial body based on a
logarithmic scale of luminosity.
Magnitude scale:
1 is 2.5:1
2 is 6.3:1
5 is 100:1
Absolute magnitude:
Equivalent to the apparent
magnitude if star were
placed 10 parsecs (32.6 light
years) from sun.
NATS 1311 From the Cosmos to Earth .
NATS 1311 From the Cosmos to Earth .
REGIONS OF SUN
Photosphere:
Bright disk
Chromosphere:
Thin, tenuous layer right above
photosphere, several thousand km
thick
Corona:
Rarefied outer region of sun's
atmosphere, millions of km thick
NATS 1311 From the Cosmos to Earth .
FEATURES OF THE SUN
Photosphere
Granules
Mottled texture of surface caused by
convection of hot gases
Gases flowing out - brighter areas
Gases flowing in - darker areas
NATS 1311 From the Cosmos to Earth FIG. 12.4
Figure 12.4
The basic
structure of
the Sun.
NATS 1311 From the Cosmos to Earth FIG. 12.2
Figure 12.2
Gravitational
equilibrium in
the Sun: At
each point
inside, the
pressure
pushing up
balances the
weight of the
overlying layers.
NATS 1311 From the Cosmos to Earth .
FEATURES OF THE SUN
Photosphere
Granules
Mottled texture of surface caused by
convection of hot gases
Gases flowing out - brighter areas
Gases flowing in - darker areas
Sun spots
Dark areas - size of earth
Average lifetime of 6 days
Regions of strong magnetic field
NATS 1311 From the Cosmos to Earth FIG. 12.3
Figure 12.3 This
photo of the
visible surface of
the Sun shows
several dark
sunspots.
NATS 1311 From the Cosmos to Earth FIG. 12.17
Figure 12.17
(a) This graph
shows how the
number of sunspots
on the Sun
changes with time.
Note the
approximately 11year cycle.
(b) This graph
shows how the
latitudes at which
sunspot groups
appear tend to shift
during a single
sunspot cycle.
NATS 1311 From the Cosmos to Earth FIG. 12.10
Figure 12.10
Granulation of the
photosphere is
evident in this
photo of two
sunspots. Each
white granule is
the top of a rising
column of hot
gas. At the darker
lines between the
granules, cooler
gas is descending
below the
photosphere.
NATS 1311 From the Cosmos to Earth FIG. 12.13
Figure 12.13
Pairs of
sunspots are
connected by
tightly
wound
magnetic
field lines.
NATS 1311 From the Cosmos to Earth FIG. 12.18
Figure 12.18 The Sun rotates more quickly at its equator
than it does near its poles, a behavior known as differential
rotation. Because gas circles the Sun faster at the solar
equator, it drags the Sun's north-south magnetic field lines
into a more twisted configuration. The magnetic field lines
linking pairs of sunspots, depicted here as green and black
blobs, trace out the directions of these stretched and
distorted field lines.
NATS 1311 From the Cosmos to Earth .
Chromosphere
Spicules
Spiked nature of chromosphere
Prominences
Rosy tongues of gas up to 30,000 km high
Chromospheric gases seen in corona
Plages
Bright areas near sunspot regions
Hotter gases
NATS 1311 From the Cosmos to Earth FIG. 12.14
Figure 12.14 This photo shows a large solar prominence,
many times the size of Earth, which consists of glowing
gas trapped by magnetic field lines arching high above the
surface of the Sun.
NATS 1311 From the Cosmos to Earth .
Flares
Brighter areas in plages
Emit radiation in x-ray band
Disrupt radio communications
Cause aurora
Corona
Solar wind
Streaming electrons and ions originating from
Corona regions called coronal holes.
NATS 1311 From the Cosmos to Earth FIG. 12.16
Figure 12.16 An X-ray image of the Sun reveals the corona:
Brighter regions of this image correspond to regions of stronger
X-ray emission. (Because X rays do not penetrate Earth's
atmosphere, photos like this one must be taken from space.)