John Grotzinger ’79, who serves as the mission leader and project scientist in charge of the recently-launched Mars Science Laboratory, was quoted in a New York Times article about the Curiosity Rover a week before its scheduled precarious landing. The article explains the Curiosity’s landing, in which “the spacecraft must flawlessly execute a series of complex maneuvers to land the rover on the surface,” as well as its mission to find evidence that the planet could have supported microbial life.
In the article, Grotzinger explains why Curiosity is to land at the Gale Crater. “Water flows downhill, and that’s where we’re going,” he says.
Grotzinger is the Fletcher Jones Professor of Geology at the California Institute of Technology. He is an eminent sedimentologist and stratigrapher with wide-ranging interests in sedimentary processes, geobiology, and Earth’s early history. He previously served as the Shrock Professor of Earth Sciences and Director of the Earth Resources Laboratory at M.I.T.
As one of only 28 scientists chosen by NASA to participate in the 2003 Mars Exploration Rover Mission, he performed an analysis of Martian sediments and sedimentary rocks and assessed the role of liquid water in shaping Martian landforms.
Grotzinger was elected into the National Academy of Sciences, one of the highest honors that can be accorded a U.S. scientist. He has also been awarded the National Science Foundation Young Investigator Award, the Fred Donath Medal from the Geological Society of America, the Henno Martin Medal from the Geological Society of Namibia, and the Charles Doolittle Walcott Medal by the National Academy of Sciences.
At Hobart, Grotzinger earned a B.S. in geoscience and was a member of the lacrosse team. He earned an M.S. from the University of Montana and a Ph.D. from Virginia Polytechnic Institute and State University. He returned to the Colleges as a Druid lecturer in 1996.
The full New York Times article about Curiosity follows.
The New York Times
A Drop-In Looking for Signs of Company
Kenneth Chang • July 30, 2012
Right now, a spacecraft containing Curiosity – a car-size, nuclear-powered planet rover – is coasting at 8,000 miles per hour toward Mars, nearing the end of a journey that began in November. With tightening budgets, it is the last big hurrah for NASA’s planetary program for quite a few years. Packed with ingenious new instruments, the rover promises to provide the best-ever examination of the Red Planet, digging up clues to a profound question: Could there ever have been life there?
Over the coming week, the pull of gravity will accelerate the spacecraft to 13,000 miles per hour, and early Monday morning Eastern Daylight Time, it is scheduled to execute a series of astoundingly complicated maneuvers and place the rover on the surface. Its new home will be the Gale Crater, just south of the equator, a 96-mile-wide bowl punched out by a meteor more than 3.5 billion years ago. It is one of the lowest places on Mars, which should help advance Curiosity’s $2.5 billion mission: studying the environment of early Mars.
“Water flows downhill, and that’s where we’re going,” John P. Grotzinger, a professor of geology at the California Institute of Technology who serves as the mission’s project scientist, said during a news conference this month.
Bits of the Martian past may lie in the rocks at the bottom of the crater. Over the past decade, NASA’s robotic spacecraft have turned up convincing evidence that eons ago the planet held one of the prerequisites for life. Water flowed on Mars, at least on occasion.
Life’s other prerequisites are carbon-based molecules and energy. Sunshine or volcanic heat could have provided the necessary energy. With Curiosity, the search is on for the carbon-based molecules.
“I think this is the Hubble Space Telescope of Mars exploration,” said John M. Grunsfeld, NASA’s associate administrator in charge of the science mission directorate. (He is best known as the Hubble repairman, flying on three space shuttle missions to refurbish and upgrade the telescope.) “This is the first time that we have a real analytical laboratory heading to the surface.”
But before Curiosity can make any discoveries, it has to land.
In the control room at NASA’s Jet Propulsion Laboratory in Pasadena, Calif., it will still be Sunday evening when the nervous wait begins. First will come word that the spacecraft containing Curiosity has entered the Martian atmosphere. Just seven minutes later, the spacecraft must flawlessly execute a series of complex maneuvers to land the rover on the surface.
If all goes as planned, the friction of Mars’ thin air rushing past the heat shield will have slowed the spacecraft to 1,000 miles per hour. A 51-foot-wide parachute will pop out, generating up to 65,000 pounds of drag force. Then the heat shield will pop off so that the radar can find the landing site in Gale Crater.
Even with the parachute drag, the spacecraft will be barreling toward the surface at 200 miles per hour. Next it will cut away the parachute and ignite its descent engines to slow down further.
The last three NASA rovers – Sojourner in 1997 and Spirit and Opportunity in 2004 – had similar landing systems, except for the final step. For those three, a cocoon of air bags inflated around the rover, which was then dropped the last 50 feet or so, bouncing and rolling until it came to a stop.
But Curiosity, about the size of a Mini Cooper, is five times as heavy as Spirit or Opportunity, making air bags impractical. It would be equivalent of trying to cushion a car hitting a brick wall at highway speed without any damage to the car.
Instead, Curiosity will be lowered by cable all the way to the ground from the hovering rocket stage in what NASA calls a sky crane maneuver. Once Curiosity bumps into Mars at a gentle 1.7 miles per hour, the cable will be cut, and the rocket stage will fly off to crash about a third of a mile away.
“Is it crazy?” Doug McCuistion, director of NASA’s Mars exploration program, asked rhetorically during the news conference. “Well, not so much. Once you get comfortable, once you understand it, it’s not a crazy concept.”
The NASA engineers who devised the sky crane maneuver say that after thorough testing of the different parts of the system and numerous computer simulations, they are confident that they have built something that will work.
“In the simulated world, we’ve landed on Mars millions of times,” one of the engineers, Steven Lee, said in an interview. “I’m actually very comfortable. I’m more comfortable with the impending landing than I was with the launch.”
Still, success is not guaranteed. The Curiosity landing is the “hardest NASA robotic mission ever attempted,” Dr. Grunsfeld said.
If it survives, Curiosity will come to rest about 1:17 a.m. Eastern Daylight Time. NASA’s Mars Odyssey orbiter will be passing overhead, in position to relay radio transmissions from Curiosity to Earth. About 14 minutes later, the fate of Curiosity may be known at mission control. (NASA warns that with the vagaries of space communications, a day or two could pass before confirmation of a successful landing reaches Earth.)
Engineers and scientists will spend several weeks checking out the condition of the rover. A few photographs will be beamed back the first few days, first in black and white, then in color. One of the first chores will be a software upgrade for Curiosity’s computers. The first drive is most likely more than a week after landing. The first flexing of the rover’s robotic arm would occur after that.
“In a couple of months, we’ll be on the road to Mount Sharp,” said Dr. Grotzinger, the project scientist.
For reasons no one can quite explain, a three-mile-high mountain, Aeolis Mons, stands at the center of Gale Crater. Informally known as Mount Sharp, in honor of Robert P. Sharp, a pioneering planetary scientist at Caltech, it is taller than any mountain in the continental United States. Orbiting spacecraft have already observed that Mount Sharp consists of layered rocks presumably formed out of sediment that settled at the bottom of Gale over millions of years. Later the sediment was somehow scoured out, leaving Mount Sharp at the center.
The layers, scientists believe, will provide a history book about early Mars. Orbiters have spotted at the base of the mountain signs of clays – minerals that form in the presence of water and that point to an environment that was less acidic than present-day Mars. As Curiosity crawls up the mountain, it will roll across younger and younger rocks, and the changes could tell how the environment of Mars changed.
For that task, Curiosity is carrying some of the most sophisticated science tools ever devised. A rock-vaporizing laser called ChemCam can turn a smidgen of rock into a puff of glowing, superhot gas from a distance of up to 25 feet. From the colors of light emitted by the gas, ChemCam can identify elements in the rock. A rock full of carbon, for example, would merit a closer look.
“It is really designed to be a sentry or advance guard for the rover and identify the most interesting samples,” said Roger C. Wiens, a physicist at Los Alamos National Laboratory who is the instrument’s principal investigator. ChemCam can also vaporize dust on a rock to get a better look at its surface.
Other instruments include a weather station; a device that shoots particles into the rock and measures X-rays coming out; and several cameras, including one that mimics the hand lens of a geologist for close-up looks at rocks. The size of a microwave oven, the biggest and probably most ambitious of the instruments is called Sample Analysis at Mars – Sam for short.
Sam contains 74 cups for studying ground-up rock. Most samples will be heated to 1,800 degrees, and three different instruments will be used to identify what gases are released, including the possibility of carbon-based molecules known as organics.
Confusingly, organic molecules can arise from nonliving chemical reactions, so the presence of organics would not prove the existence of life. Rather, the discovery of such molecules would add to the possibility of life on Mars long ago – or perhaps even today.
This will be the first search for organics since NASA’s two Viking landers in 1976. The two Vikings saw no signs of organics, which led to the dispiriting conclusion that there was no possibility of life ever on Mars. (A separate experiment did have results consistent with the existence of microbes in the soil, but most scientists concluded that it was the result of some odd, nonliving chemical reactions.)
New research a couple of years ago, however, suggested that the presence in the soil of chemicals known as perchlorates could have destroyed all of the organic molecules as the samples were being heated, thus giving misleading results. The Phoenix Mars lander discovered perchlorates in the Martian soil near the north pole in 2008.
Sam’s ovens are hotter than the ones on the Vikings and should destroy the perchlorates before they destroy the organics, said Paul R. Mahaffy, the principal investigator of the Sam instrument. In addition, nine of the cups include a chemical solvent that would allow analysis at lower temperatures.
Sam will also analyze the atmosphere, possibly confirming controversial claims that it contains methane. Methane, broken apart by sunlight and chemical reactions, lasts only a few centuries. If there is methane in Mars’s atmosphere, something must be making it – perhaps microbes.
The main mission is scheduled to last two years. Then again, the last two rovers, Spirit and Opportunity, were designed for only three months of exploration. Spirit lasted six years, and Opportunity is still rolling.
Unlike the earlier rovers, Curiosity is powered by plutonium, generating electricity from the heat of radioactive decay. It is the same type of power supply that the two Voyager spacecraft traveling at the distant reaches of the solar system have been running on for nearly 35 years.
If Curiosity lands successfully, it, too, could operate for decades.
“I’m on the edge of my seat,” Dr. Grunsfeld said. “I’m not going to sit back until it’s safely on Mars.”