Formerly known as 1999 RQ36, the space rock was chosen by process of elimination as the destination for the UA-led OSIRIS-REx mission, which will pick up a sample of its regolith and return it to Earth for analysis. Launch is little more than two months away.
Carl Hergenrother fingers a stack of white, 8½- by 11-inch paper that sits before him on his desk. As he flips through the inch-thick dossier, lines of type are clearly visible.
“This is everything we know about Bennu,” says Hergenrother, glancing down at the pile of paper.
Hergenrother is a staff scientist at the University of Arizona’s Lunar and Planetary Laboratory. Bennu is an asteroid and a small but distinct resident of our solar system — so distinct that it was chosen as the destination for the OSIRIS-REx mission.
The OSIRIS-REx spacecraft is set to launch in September and in 2020 pick up a sample of the asteroid’s regolith, the loose soil and rocky material found on its surface. The sample then will be returned to Earth for analysis.
Scientists discovered Bennu on Sept. 11, 1999, by using electro-optical telescopes operated by the Massachusetts Institute of Technology Lincoln Near-Earth Asteroid Research, or LINEAR, program. The asteroid originally was known as 1999 RQ36.
Hergenrother played a key role in choosing Bennu for the OSIRIS-REx mission. The first time he laid eyes on the asteroid, it was 2005, and 1999 RQ36 was cruising close to the Earth as it does every six years. Through the Kuiper telescope on Mount Bigelow, Bennu appeared as no more than a dot of light, “like a star that moves,” Hergenrother says.
After all, an asteroid is simply a “rock in space,” he says.
Not Your Average Space Rock
But in many ways, Bennu is a special rock.
It was 2004 when the late Michael Drake, director of the Lunar and Planetary Lab, proposed securing a sample of a near-Earth asteroid. But back then, no one knew much about Bennu. In fact, researchers were considering an assortment of other asteroids, specifically ones rich in carbon.
“We want to go to a particular type of asteroid, a carbonaceous asteroid,” Hergenrother says. Researchers also want that asteroid to be rich in volatiles — substances that boil off easily, like water.
“The thinking is that these are the kinds of objects that in the early days of the solar system seeded the Earth with the organics that life formed from, as well as the water needed,” says Hergenrother, cautioning that there is still some debate about the matter.
“But we hope that Bennu is what we would call a time capsule, that it hasn’t changed much over the history of the solar system and will show what materials looked like in the very early days of solar system.”
Hergenrother became Bennu’s champion after years of data collection and analysis — and a good deal of deductive reasoning. He served as coordinator for the mission, but much of the observation and deduction fell to other mission scientists.
“We’re now approaching a million known asteroids,” Hergenrother says. “That wasn’t the case when we started doing this 12 years ago. But we were still talking hundreds of thousands of asteroids at that time.”
However, the researchers didn’t have to analyze nearly so many. Most of them could be quickly eliminated by their stark faults, such as residing too far from Earth. Closer asteroids allow for the completion of a mission within a reasonable amount of time. That criterion alone left only a couple thousand asteroids that remained viable candidates for exploration, Hergenrother says.
And of those, many have orbits that are less than stellar.
“They’re too far from the sun or too close to the sun,” Hergenrother says. “Or they’re at a sharp angle to the Earth, which would take a more powerful rocket to get into that kind of orbit.”
Looking for ‘Favorable Orbits’
Which, in turn, left only a few hundred objects that have favorable orbits — that is, ones residing near the Earth and remaining a favorable distance from the sun. However, most of those objects are too tiny.
“Some are as small as a desk,” Hergenrother says. “The ones smaller than about 200 meters have a habit of rotating very fast. The fastest ones we know about rotate about every 16 seconds.”
That’s too fast to accommodate a spacecraft looking for a sample of regolith.
But Bennu rotates only once every 4.3 hours, slow enough to sample its regolith.
“So, once you eliminate the small guys, you look at the bigger ones that have very Earth-like orbits,” Hergenrother says. “Now you’re talking only dozens of candidates, and we wanted to go to one that’s carbonaceous.”
Which Bennu seems to be. Its carbonaceous nature sent it to the top of the list of asteroids, says Hergenrother, who emailed Drake and Dante Lauretta, saying, “Guys, this is carbonaceous. It’s looking good. And there’s radar data.”
Lauretta, professor of planetary science and cosmochemistry at the Lunar and Planetary Laboratory, is Drake’s successor as the principal investigator for the OSIRIS-REx mission.
The data showed Bennu having a polar diameter of 508 meters, a mean diameter of 492 meters and an orbital velocity of more than 28 km per second. It also showed that the asteroid has a spinning-top shape; that is, it sports a bulge along its equator, a common feature among near-Earth asteroids.
“What we think this means is that this is a rubble-pile object,” Lauretta says, meaning that Bennu probably is made out of many boulders tens to hundreds of meters across.
The boulders “are loose, and they’re responding to the forces of the asteroid spinning, and material is migrating from the pole of the asteroid and accumulating at the equator and building up a ridge,” Lauretta says.
Life Expectancy: 10 Million More Years
For better or worse, Bennu has an unstable orbit. That means it probably won’t last more than 10 million years before it collides with Earth or another planet, or falls into the sun, according to Lauretta.
This is a concern to scientists. In fact, Bennu is considered a potentially hazardous object and has a relatively high possibility of impacting the Earth. So scientists are interested in understanding how asteroids’ orbits evolve.
Key to that evolution is something known as the Yarkovsky effect.
“Which is simply that an asteroid receives energy from the sun, turns that energy into heat, and as it rotates into the afternoon throws that energy back into space as thermal energy, and that acts like a thruster and changes the orbit of the asteroid slowly but surely over time,” Lauretta says. “If you want to know where an asteroid is going to be in the future, particularly in our future, then you want to know about the Yarkovsky effect.”
Looking back on his quest to help select an asteroid suitable for sampling, Hergenrother says he sometimes thinks about what if there were no Bennu.
“There are only three carbonaceous objects that are easy to get to,” he says. “They all seem to be the same shape. They all seem to be relatively safe targets. They’re scientifically interesting, and they’re easy to get to. But that’s only three out of nearly a million.”
– By Robin Tricoles
*Source: The University of Arizona