- An asteroid impact likely caused the mass extinction that killed the dinosaurs 65 million years ago. Evidence for this comes from a thin global layer containing the rare element iridium found above the last dinosaur fossils.
- In 1994, comet Shoemaker-Levy 9 broke apart and collided with Jupiter, providing a dramatic example of a major impact event. Several black scars were left on Jupiter's atmosphere.
- While impacts from asteroids and comets are rare, the threat is real as shown by impacts to Jupiter. Near-Earth objects occasionally collide with Earth with potentially catastrophic effects.
3. 12.1 Asteroids and Meteorites
• Our goals for learning:
– What are asteroids like?
– Why is there an asteroid belt?
– How are meteorites related to asteroids?
5. • Asteroids are rocky leftovers of planet formation.
• The largest is Ceres, diameter ~1000 kilometers.
• 150,000 in catalogs, and probably over a million with
diameter >1 kilometer.
• Small asteroids are more common than large asteroids.
• All the asteroids in the solar system wouldn't add up to
even a small terrestrial planet.
Asteroid Facts
7. Asteroids with Moons
• Some large
asteroids have
their own moon.
• Asteroid Ida has a
tiny moon named
Dactyl.
8. Density of Asteroids
• Measuring the orbit
of asteroid's moon
tells us an asteroid's
mass.
• Mass and size tell us
an asteroid's density.
• Some asteroids are
solid rock; others are
just piles of rubble.
9. Asteroid Orbits
• Most asteroids orbit
in the asteroid belt
between Mars and
Jupiter.
• Trojan asteroids
follow Jupiter's orbit.
• Orbits of near-Earth
asteroids cross
Earth's orbit.
11. Thought Question
Why are there very few asteroids beyond Jupiter's
orbit?
A. There was no rocky material beyond Jupiter's orbit.
B. The heaviest rocks sank toward the center of the solar
system.
C. Ice could form in the outer solar system.
D. A passing star probably stripped away all of those
asteroids, even if they were there at one time.
12. Thought Question
Why are there very few asteroids beyond Jupiter's
orbit?
A. There was no rocky material beyond Jupiter's orbit.
B. The heaviest rocks sank toward the center of the solar
system.
C. Ice could form in the outer solar system.
D. A passing star probably stripped away all of those
asteroids, even if they were there at one time.
14. Thought Question
Which explanation for the belt seems the most
plausible?
A. The belt is where all the asteroids happened to form.
B. The belt is the remnant of a large terrestrial planet that
used to be between Mars and Jupiter.
C. The belt is where all the asteroids happened to survive.
15. But WHY didn't they
form a planet?
Thought Question
Which explanation for the belt seems the most
plausible?
A. The belt is where all the asteroids happened to form.
B. The belt is the remnant of a large terrestrial planet that
used to be between Mars and Jupiter.
C. The belt is where all the asteroids happened to
survive.
16. Orbital Resonances
• Asteroids in
orbital resonance
with Jupiter
experience
periodic nudges.
• Eventually, those
nudges move
asteroids out of
resonant orbits,
leaving gaps in
the asteroid belt.
17. Origin of Asteroid Belt
• Rocky
planetesimals
between Mars and
Jupiter did not
accrete into a
planet.
• Jupiter's gravity,
through influence of
orbital resonances,
stirred up asteroid
orbits and
prevented their
accretion into a
planet.
21. Meteorite Types
1) Primitive: unchanged in composition since they
first formed 4.6 billion years ago
2) Processed: younger; have experienced
processes like volcanism or differentiation
24. Meteorites from Moon and Mars
• A few meteorites arrive from the Moon and
Mars.
• Composition differs from the asteroid fragments.
• A cheap (but slow) way to acquire Moon rocks
and Mars rocks
25. What have we learned?
• What are asteroids like?
– They are rocky, small, potato-shaped
leftovers from the era of planet formation.
• Why is there an asteroid belt?
– Orbital resonances with Jupiter prevented
planetesimals between Jupiter and Mars from
forming a planet.
26. What have we learned?
• How are meteorites related to asteroids?
– Primitive meteorites are remnants from solar
nebula.
– Processed meteorites are fragments of larger
bodies that underwent differentiation.
27. 12.2 Comets
• Our goals for learning:
– What are comets like?
– Where do comets come from?
29. Comet Facts
• Formed beyond the frost line, comets are icy
counterparts to asteroids.
• Nucleus of comet is a "dirty snowball."
• Most comets do not have tails.
• Most comets remain perpetually frozen in the
outer solar system.
• Only comets that enter the inner solar system
grow tails.
31. Nucleus of Comet
• A "dirty snowball"
• Source of
material for
comet's tail
32. Deep Impact
• Mission to study
nucleus of Comet
Tempel 1
• Projectile hit
surface on July 4,
2005.
• Many telescopes
studied aftermath
of impact.
33. Anatomy of a Comet
• A coma is the
atmosphere that
comes from a
comet's heated
nucleus.
• A plasma tail is gas
escaping from
coma, pushed by
the solar wind.
• A dust tail is pushed
by photons.
38. • Only a tiny number of
comets enter the inner
solar system. Most
stay far from the Sun.
• Oort cloud:
on random orbits
extending to about
50,000 AU
• Kuiper belt:
on orderly orbits from
30–100 AU in disk of
solar system
39. How did they get there?
• Kuiper belt comets formed in the Kuiper belt: flat
plane, aligned with the plane of planetary orbits,
orbiting in the same direction as the planets
• Oort cloud comets were once closer to the Sun,
but they were kicked out there by gravitational
interactions with jovian planets: spherical
distribution, orbits in any direction
40. What have we learned?
• What are comets like?
– Comets are like dirty snowballs.
– Most are far from Sun and do not have tails.
– Tails grow when comet nears Sun and
nucleus heats up.
• Where do comets come from?
– Comets in plane of solar system come from
Kuiper belt.
– Comets on random orbits come from Oort
cloud.
41. 12.3 Pluto: Lone Dog No More
• Our goals for learning:
– How big can a comet be?
– What are the large objects of the Kuiper
belt like?
43. Pluto's Orbit
• Pluto will never hit Neptune, even though their orbits
cross, because of their 3:2 orbital resonance.
• Neptune orbits three times during the time Pluto orbits
twice.
44. Is Pluto a Planet?
• Much smaller than the terrestrial or jovian
planets
• Not a gas giant like other outer planets
• Has an icy composition like a comet
• Has a very elliptical, inclined orbit
• Has more in common with comets than with the
eight major planets
45. Other Icy Bodies
• There are many icy
objects like Pluto on
elliptical, inclined
orbits beyond
Neptune.
• The largest of these,
Eris, was discovered
in summer 2005, and
is even larger than
Pluto.
46. Kuiper Belt Objects
• These large, icy
objects have orbits
similar to the smaller
objects in the Kuiper
belt that become
short period comets.
• So are they very
large comets or very
small planets?
47. What are the large objects of the Kuiper belt
like?
48. What is Pluto like?
• Its moon Charon is nearly as large as Pluto itself
(probably made by a major impact).
• Pluto is very cold (40 K).
• Pluto has a thin nitrogen atmosphere that will
refreeze onto the surface as Pluto's orbit takes it
farther from the Sun.
50. Other Kuiper Belt Objects
• Most have been discovered very recently so little
is known about them.
• NASA's New Horizons mission will study Pluto
and a few other Kuiper belt object in a planned
flyby.
51. Pluto and Eris
• Pluto's size was overestimated after its
discovery in 1930, and nothing of similar size
was discovered for several decades.
• Now other large objects have been discovered in
Kuiper belt, including Eris.
• The International Astronomical Union (IAU) now
classifies Pluto and Eris as dwarf planets.
• Dwarf planets have not cleared most other
objects from their orbital paths.
52. What have we learned?
• How big can a comet be?
– The Kuiper belt from which comets come
contains objects as large as Pluto.
• What are the large objects of the Kuiper
belt like?
– Large objects in the Kuiper belt have orbits
and icy compositions like those of comets.
53. 12.4 Cosmic Collisions: Small Bodies
Versus the Planets
• Our goals for learning:
– Have we ever witnessed a major impact?
– Did an impact kill the dinosaurs?
– Is the impact threat a real danger or media
hype?
– How do the jovian planets affect impact
rates and life on Earth?
55. • Comet SL9 caused a string of violent impacts on Jupiter
in 1994, reminding us that catastrophic collisions still
happen.
• Tidal forces tore it apart during a previous encounter with
Jupiter.
56. • An impact plume
from a fragment of
comet SL9 rises
high above
Jupiter's surface.
Photo Credit: HST Jupiter Imaging Science Team
61. Mass Extinctions
• Fossil record shows occasional large dips in the
diversity of species: mass extinctions.
• Most recent was 65 million years ago, ending
the reign of the dinosaurs.
62. Iridium: Evidence of an Impact
• Iridium is very rare in Earth surface rocks but
often found in meteorites.
• Luis and Walter Alvarez found a worldwide layer
containing iridium, laid down 65 million years
ago, probably by a meteorite impact.
• Dinosaur fossils all lie below this layer.
63. Dinosaur fossils in
lower rock layers
No dinosaur fossils in
upper rock layers
Thin layer containing
the rare element
iridium
Iridium Layer
64. Consequences of an Impact
• Meteorite 10 kilometers in size would send large
amounts of debris into atmosphere.
• Debris would reduce sunlight reaching Earth's
surface.
• Resulting climate change may have caused
mass extinction.
65. Likely Impact Site
• Geologists have
found a large
subsurface
crater about 65
million years old
in Mexico.
66. Likely Impact Site
• A comet or
asteroid
about 10
kilometers in
diameter
approaches
Earth.
72. Facts about Impacts
• Asteroids and comets have hit Earth.
• A major impact is only a matter of time: not IF
but WHEN.
• Major impacts are very rare.
• Extinction level events happen millions of years
apart.
• Major damage happen tens to hundreds of years
apart.
74. • Crater made by the impact of a 1–2 meter object
in Peru, 2007
75. Frequency of Impacts
• Small impacts
happen almost
daily.
• Impacts large
enough to
cause mass
extinctions
happen many
millions of years
apart.
76. The asteroid with our name on it
• We haven't seen it yet.
• Deflection is more probable with years of
advance warning.
• Control is critical: Breaking a big asteroid into a
bunch of little asteroids is unlikely to help.
• We get less advance warning of a killer comet….
77. What are we doing about it?
• Stay tuned to
http://impact.arc.nasa.gov
78. How do the jovian planets affect impact
rates and life on Earth?
79. Influence of the Jovian Planets
• Gravity of a jovian planet (especially Jupiter) can redirect
a comet.
80. Influence of Jovian Planets
• Jupiter has directed some comets toward Earth but has
ejected many more into the Oort cloud.
81. • Was Jupiter necessary
for life on Earth?
• Impacts can extinguish life.
• But were they necessary
for "life as we know it"?
82. What have we learned?
• Have we ever witnessed a major impact?
– The most recent major impact happened in
1994, when fragments of comet SL9 hit
Jupiter.
• Did an impact kill the dinosaurs?
– Iridium layer just above dinosaur fossils
suggests that an impact caused mass
extinction 65 million years ago.
– A large crater of that age has been found in
Mexico.
83. What have we learned?
• Is the impact threat a real danger or media
hype?
– Large impacts do happen, but they are rare.
– They cause major extinctions about every 100
million years.
• How do the jovian planets affect impact rates
and life on Earth?
– Jovian planets sometimes deflect comets
toward Earth but send many more out to Oort
cloud.
Editor's Notes
Thought question: were these pictures taken from Earth?
Rocky material condensed everywhere.
B. The students often get confused by the differentiation ideas they've just
heard about in planet formation.
D. If a passing star ripped off asteroids, it would have stripped away comets
and planets too. (That may be one explanation for the truncation of the
Kuiper belt…)
Discussion: A -- planetesimals formed EVERYWHERE in the solar system.
B--there's not enough mass in the asteroid belt to be the remnant of even
a small terrestrial planet.
(note deleted)
Simple rocks and metal, occasionally carbon compounds and water.
Shiny bits are metal flakes, first to condense.
White features are solidified droplets of material that splashed out during impacts during accretion
Simple rocks and metal, occasionally carbon compounds and water.
Shiny bits are metal flakes, first to condense.
White features are solidified droplets of material that splashed out during impacts during accretion
Several atomic bombs worth of energy.
Crater is 15 meters across.
Impact spewed debris more than 300 meters and shattered windows as far as a kilometer away.