As the asteroid Bennu comes into sharper focus, planetary scientists are seeing signs of water locked up in the asteroids rocks, NASA team members announced December 10.
“Its one of the things we were hoping to find,” team member Amy Simon of NASAs Goddard Space Flight Center in Greenbelt, Md., said in a news conference at the American Geophysical Union meeting in Washington, D.C. “This is evidence of liquid water in Bennus past. This is really big news.”
NASAs OSIRIS-REx spacecraft just arrived at Bennu on December 3 (SN Online: 12/3/18). Over the next year, the team will search for the perfect spot on the asteroid to grab a handful of dust and return it to Earth. “Very early in the mission, weve found out Bennu is going to provide the type of material we want to return,” said principal investigator Dante Lauretta of the University of Arizona in Tucson. “It definitely looks like weve gone to the right place.”
OSIRIS-RExs onboard spectrometers measure the chemical signatures of various minerals based on the wavelengths of light they emit and absorb. The instruments were able to see signs of hydrated minerals on Bennus surface about a month before the spacecraft arrived at the asteroid, and the signal has remained strong all over the asteroids surface as the spacecraft approached, Simon said. Those minerals can form only in the presence of liquid water, and suggest that Bennu had a hydrothermal system in its past.
Bennus surface is also covered in more boulders and craters than the team had expected based on observations of the asteroid taken from Earth. Remote observations led the team to expect a few large boulders, about 10 meters wide. Instead they see hundreds, some of them up to 50 meters wide.
“Its a little more rugged of an environment,” Lauretta said. But that rough surface can reveal details of Bennus internal structure and history.
If Bennu were one solid mass, for instance, a major impact could crack or shatter its entire surface. The fact that it has large craters means it has survived impacts intact. It may be more of a rubble pile loosely held together by its own gravity.
Telling scars[hhmc]
Crater pockmarks on Bennu, like this 20-meter-wide depression photographed on December 2, may turn out to be the safest places for the spacecraft to pick up a sample of the asteroid. Craters also tell scientists that the asteroid is not one solid mass but instead different materials clumped together. If Bennu had been a solid rock, large impacts could crack or shatter its surface.
The asteroids density supports the rubble pile idea. OSIRIS-RExs first estimate of Bennus density shows it is about 1,200 kilograms per cubic centimeter, Lauretta said. The average rock is about 3,000 kilograms per cubic centimeter. The hydrated minerals go some way towards lowering the asteroids density, since water is less dense than rock. But up to 40 percent of the asteroid may be full of caves and voids as well, Lauretta said.
Some of the rocks on the surface appear to be fractured in a spindly pattern. “If you drop a dinner plate on the ground, you get a spider web of fractures,” says team member Kevin Walsh of the Southwest Research Institute in Boulder, Colo. “Were seeing this in some boulders.”
The boulders may have cracked in response to the drastic change in temperatures they experience as the asteroid spins. Studying those fracture patterns in more detail will reveal the properties of the rocks.
The OSIRIS-REx team also needs to know how many boulders of various sizes are strewn across the asteroids surface. Any rock larger than about 20 centimeters across would pose a hazard to the spacecrafts sampling arm, says Keara Burke of the University of Arizona. Burke, an undergraduate engineering student, is heading up a boulder mapping project.
Cracked surface[hhmc]
Some of the rocks strewn across Bennu, like this 35-meter-wide boulder photographed on December 2, are fractured in a spindly pattern. The fractures may be the result of sudden, drastic temperature change. Studying the fracture patterns could help scientists learn more about the properties of the rocks.
“My primary goal is safety,” she says. “If it looks like a boulder to me, within reasonable guidelines, then I mark it as a boulder. We cant sample anything if were going to crash.”
The team also needs to know where the smallest grains of rock and dust are, as OSIRIS-RExs sampling arm can pick up grains only about 2 centimeters across. One way to find the small rocks is to measure how well the asteroids surface retains heat. Bigger rocks are slower to heat up and slower to cool down, so theyll radiate heat out into space even on the asteroids night side. Smaller grains of dust heat up and cool down much more quickly.
“Its exactly like a beach,” Walsh says. “During the day its scalding hot, but then its instantly cold when the sun sets.”
Measurements of the asteroids heat storage so far suggest that there are regions with grains as small as 1 or 2 centimeters across, Lauretta said, though it is still too early to be certain.
“I am confident that well find some fine-grained regions,” Lauretta said. Some may be located inside craters. The challenge will be finding an area wide enough that the spacecrafts navigation system can steer to it accurately.
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