Martian wandering
University of California, Berkeley: 13- There were once great oceans on Mars, say a team of scientists at the University of California, Berkeley. A large plain at the planet's north pole looks very like an ocean basin, even from Earth. Images taken by the Viking spacecraft in the 1980s showed two possible ancient shorelines. Each of these was thousands of kilometres long, with features like those found in Earth's coastal regions. These dried- But then in the 1990s Mars Global Surveyor measured the surface of Mars to a resolution of 300 metres. They found that the shorelines vary in height by several kilometres (more than a mile). They rise and fall like waves, with several thousand kilometres from one peak to the next. Here on Earth the height of any shoreline is pretty much the same everywhere. So experts began to reject the notion that Mars once had oceans. But the UC Berkeley scientists have now found an explanation for the undulating Martian shorelines. The north and south poles of Mars have moved by nearly 3,000 kilometres along its surface. This happened within the past 2 or 3 billion years. Spinning objects bulge at their equator. So this "true polar wander" could have caused the change in height of the shorelines that we now see on Mars, say the scientists. "When the spin axis moves relative to the surface, the surface deforms," says study co- The paper will appear in this week's issue of Nature. The lead author is Taylor Perron, a former UC Berkeley graduate student, now a postdoctoral fellow at Harvard University. Perron's calculations show that the response of Mars' elastic crust could create very large elevation differences for features like a shoreline. This is exactly what we see. The Arabia shoreline varies in elevation by about 2.5 kilometres. The Deuteronilus shoreline varies by about 0.7 kilometres. "This is a beautiful result that Taylor got," says co- "The mere fact that you can explain a good fraction of the information about the shorelines with such a simple model is just amazing. It's something I never would have guessed at the outset. "This really confirms that there was an ocean on Mars." So now the question is: What caused Mars' spin axis to move? A spinning planet is most stable when its mass is farthest from its spin axis. So any shift of mass on the planet could cause the spin axis to move. This might be a shift of mass within the mantle. It could be a mass shift between the mantle and the crust to form a volcano. It could even be an addition of mass caused by a meteorite hitting the planet. Richards has modelled polar wander in Earth's past. This was generated by the upwelling of hot mantle. Some scientists believe this shifted Earth's spin axis 800 million years ago, by 90 degrees, tipping the planet on its side. The UC team calculates that on Mars an initial shift of 50 degrees from today's pole would have been enough to disrupt the Arabia shoreline. This is equal to about 3,000 kilometres on the surface. A shift of 20 degrees from today's pole, or 700 kilometres, would have changed the Deuteronilus shoreline. Interestingly, today's pole and the two ancient poles lie in a line that is a constant distance from the planet's largest feature. This is the Tharsis rise, a huge bulge near the equator which contains Mars' most recent volcanic vent, Olympus Mons. Tharsis is the largest volcano in the solar system. It formed about 4 billion years ago, not long after Mars solidified. The positions in relation to each other of Tharsis and the path of the poles is exactly what scientists would expect if a mass had shifted that was smaller than the Tharsis rise. This is because the planet would then rotate so that the large mass of Tharsis stayed on the equator - as far away from the axis as possible. "This alignment is unlikely to occur by coincidence," the team writes. Manga has a hunch about the mass shift that led to the tilt of Mars' spin axis. If a flood of water had filled the Arabia ocean 3 billion years ago, to a depth of several kilometres, that might have been enough to shift it 50 degrees to the south. When the water disappeared, the pole could have shifted back again. Then it could have shifted again by 20 degrees during the flood that created the Deuteronilus shoreline. The unknown source of water must have produced a flood greater than any seen on Earth, Manga says. Huge canyons have been cut in the flanks of the Tharsis rise. Where has the water gone? Well it might have evaporated. But there is another, more intriguing possibility. All that water might have sunk into underground dikes. These would be frozen near the surface. But they could be liquid below. More help with words conference core depression doctorate erupt journal lava orbit planet vapour research volcanic
What's it all about?
Learning to do science is about learning to think. Experiments, direct teaching, group activities and discussions all have a part to play. So do science news stories.
Like other non-fiction texts, science stories contain different kinds of statements. To get at the science behind the words -
All these types of statement occur in some science stories. Virtually all science stories, however, will contain statements of the following four types:
- new findings or developments;
- the technology and methods the scientists used;
- previous or accepted knowledge, which may or may not be supported by the new findings;
- issues, implications and applications of the research.
So the next activity is designed to engage students with the latest science news by exploring the meaning and structure of a story as revealed by the content and balance of these four statement types:
Pulling it apartIn groups students should read through the story looking for new findings or developments. Once they have reached agreement, or at least consensus, and have underlined all the statements about what the scientists have just discovered or achieved, they can compare and discuss.
In groups they should go through the story again looking for the technology and methods the scientists used in their research. Once they have reached agreement or consensus, and have underlined the statements that talk about the methods and equipment the scientists used, they can compare and discuss.
They should repeat the activity for existing knowledge.
Any areas of disagreement in these activities - whether among the students or between teacher and students - should be regarded as opportunities for discussion rather than errors to be corrected.
Having fully engaged with the latest science news through the above activities, students will be far better able to talk and think about the science and its implications than someone who has simply read about it in a newspaper or watched a brief item on television.
Now it's time for them to get to grips with the issues raised by the research.
Young people have opinions. But school science traditionally allowed little scope for forming and expressing these - which is why it turned many of them off the subject for life.
Putting it together again
In groups, students should read through the latest story looking for issues, implications and applications. Once they have reached agreement, or at least consensus, and have underlined all the relevant statements in the story, they can compare and discuss.
Having done all this the students are well armed to explore the issues raised by the story. A suggested discussion topic specific to this new story is provided below.
Topic for discussion, research or pupil presentations A simple demonstration of a spin axis shifting can be done with a football and a lump of something sticky, like wet mud or honey. If the football is set spinning on the floor with its axis straight up, and the sticky stuff dropped in the region of its "north pole" what happens next simulates how the spin axis of Mars has shifted, according to the UC scientists. Two things to notice, the second not obvious from the story: 1) The sticky stuff ends up going around the equator. 2) It is not the spin axis that shifts, but the planet with respect to the axis. The orientation of the spin axis in space is fixed (apart from the effect of the small torque of the incoming mass), but the positions of the poles on the planet move. Working in groups pupils should predict what will happen, do the experiment, then compare their predictions with what actually happened. They should then try to explain what they saw. It takes a bit of teacher practice to get the spin rate and stickiness just right, so that big blobs of honey don't go flying around the room - A less messy approach would be to use the teaching aid movie on polar wander set up by Dave Stegman at Monash University Teachers can find more activities, resources and lessons about Mars here Tips for science class discussions and groupwork No 52 "The 5- For those that like every class at the same point every day, this can be a hard item to deal with." For more see 5E model and constructivism.
For myself, I find it exciting to develop lessons where I get to be creative and I can keep the creativity in my classroom. Personal opinion, but I think that as we move students through to graduation, we are being forced to take the creativity out of their learning experience. The 5-
NSTA forum entry by teacher Bob Penrose (May 2007)
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