Introduction to the Solar System
APAS 1110 Summer 2000
Earth-Venus-Mars: The Evolution of Landscape
Thursday, June 15
Lecturer: Mark Bullock
• SLIDE: Mercury
Mariner 10 in 1974 -- only spacecraft to visit
Very moonlike, old surface, many craters
Mercury has a large iron core 3/4 diameter
Exciting news-- may be ice at the poles, in the shadows of craters that never see light. Ice would have stayed after a comet impact. The same thing may even be true of our Moon
No atmosphere
• SLIDE: Faults on Mercury
After Mercury had collected craters, caused by leftover planetesimals, it apparently shrank 2-4 km in diameter. Stresses on its crust--made huge faults where one part of the crust tried to ride up onto another, almost like plate tectonics. Due to cooling of planet and formation of core
• SLIDE: Venus in a Telescope
Much of the solar system was explored in the 60’s, 70’s and 80’s (Pioneer, Voyager, Viking).
Venus remained an enigma because of its global sulfuric acid cloud cover
Exception: Soviet exploration included landers on Venus that imaged the surface
• SLIDE: Magellan
Cobbled together from old spare Voyager parts, the spacecraft that had been sent out earlier to Jupiter, Saturn, Uranus and Neptune
Launched 1989
Had only one instrument, an imaging radar system
Radar has wavelength of 4 cm, and can see through the cloud
Mapped the whole planet, things as small as 200 m
• SLIDE: Data Comparing Venus and the Earth
Venus: Earth’s twin--almost same size, composition, gravity, and distance from Sun
Venus spins backwards--maybe due to a giant impact flipping it over
Day is 117 days, but this is its synodic period --noon to noon
Sidereal day - one rotation with respect to stars, is 243 days
Its year is 225 days. Year is less than its day
Very, very hot, heavy atmosphere, covered in clouds
CO2, N2 atmosphere
• SLIDE: Venus, Earth Topography
Venus is way too hot to have liquid or solid water -- but there’s a tiny bit in the atmosphere. So it doesn’t have oceans
But it has large, continent like features, and low lying volcanic plains
Recall that there is a compositional difference between oceanic and continental crust
Is the same true for Venus--are the highlands lighter rocks floating on heavier rocks?
Is there plate tectonics on Venus?
• SLIDE: How Radar Works
Sends out radio pulses
They bounce off rocks, some rocks reflect more than others
Pulses are received, computer reconstruction of surface
Radar is not light -- bright means rough or electrically conductive
Dark means smooth or an insulator
• SLIDE: LA Basin
Here’s an image of the LA basin, using radar. Can see right through clouds, but things don’t look quite right. Mountains
Have to keep this in mind when we’re looking at Magellan Radar images
• SLIDE: Venus Mosaic 0 deg
Bright and rough continental area, Alpha Regio. Looks like scrunched up crust
Dark, patches around craters that may be related to dust kicked up from the impacts
Highest mountains -- 12 km high (40,000 ft). Very reflective, could be solidified metal, spewed out from volcanoes
• SLIDE: Venus Mosaic 90 deg
Going E around Venus, we see the beginnings of a huge continent-like area, called Aphrodite. Shot through with enormous chasms that look like giant rift zones. At first we thought that it might have been plate tectonics, but there is no evidence anywhere for subduction zones
Large circular regions may be partial subduction zones, or they may be places where huge plumes came up from the mantle, and spread out under the lithosphere. They are called coronae
• SLIDE: Venus Mosaic 270 deg
In addition to 10’s of enormous volcanoes, (600 km across, 5X bigger than Moana Loa, biggest volcano on Earth), may 10,000s of small shield volcanoes, 20 km across.
• SLIDE: Crater Farm
There are about 910 craters on Venus, none smaller than 1.5 km. This is because the atmosphere is so thick that any impactor smaller than 150 m across gets burned up. These craters formed on the volcanic plains. Notice the bright impact ejecta--rough, blocky material thrown out of the craters
• SLIDE: Crater Mead
Largest impact crater on Venus, 280 km across.
Named after Margaret Mead--all feature on Venus named after women
Except Maxwell, after James Clerk Maxwell, studied light and radio
• SLIDE: Maxwell Montes
There are lots of regions of scrunched up crust (more violent than on the Earth), called tessera. There are very few impact craters on the tessera, indicating that the surface has been so recently that the craters have been wiped out. We call this a young surface, like the Earth
• SLIDE: Lava Flooded Impact Crater
So we have only 910 craters, with maybe 34 of them modified. Venus has wiped out all the older craters, but there is no real evidence of how they got wiped out--the modified ones aren’t enough
This has yielded a theory called catastrophic resurfacing -- 500 my ago, the entire lithosphere of Venus became unstable, and reworked itself in 100 my. It turned over in one enormous burp, followed by the building up of volcanoes, and the wholesale cracking and buckling of the crust. But no plate tectonics -- that is a continual process.
• SLIDE: Pancake Domes
Upwelling of thick, viscous lava, forming these pie shaped bubbles of magma under the surface
• SLIDE: Arachnoids
Even stranger volcanic features, small volcanoes called arachnoids, because they look like spiders
You can even see a vent, and the intense tectonic fractures around it
• SLIDE: Coronae
Huge circular features, but ranging in size from 100 km to 2600 km. May be the surface expression of huge plumes from the interior, or maybe where crust is subducting slowly
Still, no global pattern of plates like we clearly see on the Earth
• SLIDE: 3-D Volcano
Magellan took three kinds of data -- images, altitudes, and gravity.
We have been looking at the images
Gravity tells us the density of stuff beneath the crust, so that we can tell if some things are continents, or if volcanoes have deep roots
Altitude tells us how high things are
If we use a computer to combine the image and altitude data, we can simulate any perspective, even ones the spacecraft never had.
This is a volcano, where you can see recent bright flows that came off the summit. The dark, smooth area is old lava flows, maybe lava plains that existed before the volcano
• SLIDE: Fracture with Crater
The same is true of craters split by fractures--there are very few
Here we see one of the many, many cracks, but only one disrupted crater.
• SLIDE: Sand Dunes
Even though Venus has a very thick atmosphere, there are only weak winds at the surface. The reason is that the air conducts the heat very efficiently, and temperature differences from place to place, that drive winds, don’t build up.
But there is some wind, and even some sand dunes. But we know it isn’t too common, because we don’t see sand all over the place, like in craters
• SLIDE: Venera 9 Surface
The Soviets were much more aggressive in sending missions to Venus
They sent a number of landers, which sent pictures for one hour (1970s)
Here’s what the surface looked like
Rocks, soil like surface, a little bit of sky
Image is distorted because of the camera optics.
Looks like a volcanic plain
• SLIDE: Channels
Another mystery of Venus is a network of channels, some 6000 km, and going uphill! They couldn’t have formed from water, because it’s too hot.
We know that it’s been hot since the catastrophic event, because there are no small craters, the air has been thick, and the greenhouse effect has prevailed
Channels might be some kind of lava tube, but there are no lava tubes on Earth anywhere near this long--long as the longest rivers on Earth
• SLIDE: River Delta
At the end of the long channels, or canali, there are river delta features
It looks like the liquid that made the channels ended its journey here, but they look a lot like terrestrial river deltas
A scientist at USGS has come up with a suggestion to explain these river delta features
They could be formed by low temperature lavas, ones that stayed liquid for a long time on the hot Venus surface, and flowed like water
He even proposed that this stuff could still be liquid, in under ground rivers of liquid carbonate
• SLIDE: Reticulate Terrain
Highly organized cracks that extend for thousands of km. The whole surface of Venus experienced huge stresses, apparently in a globally synchronous event.
One theory (mine) is that climate change, induced by volcanic release of greenhouse gases, heated and cooled the surface enough to crack it.
• SLIDE: Mars
Half the size of Earth
24 hour day, same as Earth
23 deg axial tilt, same as Earth --which means it has seasons just like Earth
Half as much sunlight as Earth
Very cold, -50 F on average
But in the summer on the equator, it can get room temperature
Has a thin CO2 atmosphere, 1/100th of the Earth’s.
Almost same composition as Venus’, but 10,000 times thinner
Has polar caps, made of water ice and dry ice (CO2)
It has weather, with morning clouds, snow, storms, dust storms
But no evidence for running water recently (recall surface dating with crater counting). It’s all frozen out.
• SLIDE: Marineris Hemisphere
Here’s what Viking saw
Mars has two kinds of terrain, roughly divided between the Northern hemisphere and Southern hemisphere
The northern hemisphere, which we are looking at here is smooth, relatively crater free
It has huge shield volcanoes, sitting on a huge bump on the surface, as well as other places.
It also has an enormous crack, the size of the US, splitting down the side of the bump
The northern hemisphere has relatively few craters, probably wiped out by the volcanism--it is a relatively young surface, maybe 1 by old
Notice the clouds on the morning terminator--morning fog surrounding three enormous volcanoes on the Tharsis bulge
Light is where windblown dust has settled -- dark areas may be bedrock
Mars is red because it the surface has oxidized iron -- rust, just like volcanic red dirt on the Earth
The southern hemisphere is much, much older, as evidenced by a lot of craters
The entire south is higher than the volcanic plains, and we call it the highlands, just like on the moon
• SLIDE: Boundary Scarp
Some people have even suggested that Mars may have had oceans, and that there are ancient shorelines
This is the scarp that makes a boundary between the south and north
you can see a crater with lobate ejecta in the center right
Channels ending between s and n
Sand dune fields
Some craters have funny impact ejecta, called lobate ejecta
It looks like the impactor hit where there was subsurface ice
The ice melted on impact, made mud, which was flung out in these patterns
• SLIDE: River Valleys
In fact everywhere we look, in both the old (South) and new (north) areas of Mars, we see evidence for running water in the past
Here is a very, very old valley network
The valleys are more common in the old regions, but there is also evidence for a large system of drainage networks from older region to newer regions
Some of the river systems clearly look like rivers, and must have carried enormous amounts of water
We interpret this to mean that Mars was warmer in the past
It has almost no greenhouse effect now, because the air is so thin
But it may have had a much thicker CO2 atmosphere in the past, now sequestered at the poles or escaped from the planet
Mars has a lower gravity, and light gases can escape easily
Higher pressure, more greenhouse, liquid water
Now the water is probably frozen as permafrost, or under the ground
There is other evidence for massive climate change as well
Water-carved channel shown here has evidence for sustained, multiple
Flow events. Notice terracing and central, smaller channel
• SLIDE: Teardrop
But there is other evidence for flowing water
Here, you see a teardrop shape around a crater. Somehow when the crater formed (before the flood) it sort of cemented the ground, making it more resistant to erosion as the water flowed
• SLIDE: Chaotic Terrain
There are places where it looks like huge amounts of ice melted suddenly and flowed out. The land collapsed in these places, creating chaotic terrain
There are places like this on the Earth -- badlands of Eastern Washington
Most of the intricate river networks are ancient -- 3.5 B years ago
Recall that the solar system is 4.5 billion years old
But there is more recent evidence of flowing water
This is the result of a series of great floods
You can tell that the water has moved fast, cutting deep channels
These may have been much more recent -- maybe 1 By ago
• SLIDE: Argyre
The southern portion looks just like the moon, like a dead planet
This is a huge basin and numerous other craters in the south
When we sent Mariner 9 there in 1971, it flew under the south pole, and we thought Mars was just like the Moon. It was very disappointing
But Viking changed all that
Layering can be seen here – evidence for multiple volcanic flows that may
Have built up this portion of the surface of Mars.
Also – landslides – can see the debris at the bottom of the canyon.
Valles Marineris definitely was not formed by water, because we don’t see any evidence of sediments
But we do see a lot of carved away cliffs, shown in this oblique image of Candor Chasma
When we look very closely at the cliffs, we see layers at the top, just like layers on the Earth
These may have been put down by volcanic events, or may be rocks that reacted with gases in the atmosphere when it was different (volcanically active)
• SLIDE: South Polar cap
The polar caps grow and shrink with the seasons
But there is a permanent core, that looks like it may have huge ice walls and canyons
This image was taken in the late summer, when the pole is lit up and about to plunge into a midnight sun, when the cap will grow
As the cap sublimates (grows or shrinks), a huge polar vortex of air is generated, circulating about the cap.
you can see how the cap get laid down by the intricate spiral pattern
• SLIDE: Polar Laminated Terrain
Because the caps might be sources of water, and give a clue to Mars’ climate, Viking looked very hard there
This is near the edge of the N polar cap, where there are probably large cliffs and canyons of ice
There are intricate lines of alternating ice and dirt.
This is evidence for climate change on Mars
There were times when ice was deposited and taken away, and times when dust or dirt was deposited or taken away
The caps have experienced a varying climate
• SLIDE: Olympus Mons
The biggest volcano in the solar system
80,000 feet high, 500 miles across
Called Olympus Mons
Enormous pit in the center
Calderas are formed when the volcano finished erupting, and the magma from below withdraws. The ground collapses at the top
Because it is so high, Olympus Mons strongly influences the weather on Mars, just like mountains do here
Here is an oblique view of the summit, encircled by clouds
Dunes composed of dark sand grains encircle the north polar cap of Mars. This view was taken during the northern summer in May 1999.
Mars Global Surveyor, Thermal Emission Spectrometer instrument (infrared).
Coarse-grained hematite (oxidized iron) near the equator of Mars. This kind
Of mineral forms on Earth in hydrothermal environments (such as Yellowstone).
These meteorites definitely came from Mars! Gases in pore spaces
Are the same composition as Mars’s atmosphere – even the isotopes are the same.
Blasted off the surface of Mars from an asteroid impact, Jupiter’s gravity
Perturbs the Mars rocks so that they fall inward toward the sun. Some
Encounter the Earth on the way in.
• SLIDE: Simulated Landing
Since we didn’t know what to expect, we surveyed possible landing sites for several months before deploying the landers
The lander used parachute and rockets, and used the orbiter as a relay
Landers were semiautonomous, and bristling with instruments
• SLIDE: Dust Storm at Surface
One thing about the wind on Mars -- it can get very strong
It can get so strong that dust storms kick up during the warmest weather in the south
Most dust storms are local, but they can all combine to cover the planet completely
Dust storms came by several times while Viking 1 sat and made its measurements for two years on the surface
This is a series of images (taken at the same time of day) showing how everything got darker during a dust storm
• SLIDE: Big Joe
Rock seen at the V1 landing site
About two meters across, called ‘Big Joe’
You can see where sand from dust storms have settled on it
But you can also see where the sand slumped off
This happened while the lander was there -- we saw it before and after
• SLIDE: Trench
Viking scooped up soil with a shovel, and put it in various chambers for testing
They tested what elements the rocks were made of -- Fe, Mg, Al --basalts
They looked for water (1%)
I know a researcher who discovered you can retrieve the water from this kind of soil with a microwave oven
• SLIDE: First Surface Photo
You can imagine the anticipation we felt, wondering what this new place, new world looked like.
Far more Earth like, this is even a place that could be home to humanity
Here’s what it saw
Rock strewn desert, light sky
The rocks are probably strewn from some distant impact crater or volcano
If you look at the rock on the lower right, it looks vesicular
That means it has evidence of bubbles that came out as the rock cooled
Probably volcanic in origin
Probably the most important thing we can learn from exploring the other planets is from a sentiment expressed by T.S. Eliot (who was neither an astronaut nor an astronomer):
"We shall not cease from exploration, and the end of all our exploring will be to arrive where we started and know the place for the first time."