[meteorite-list] Proposed Mission Will Return Sample from Near-Earth Object (OSIRIS)

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Tue, 13 Mar 2007 09:11:45 -0700 (PDT)
Message-ID: <200703131611.l2DGBk409787_at_zagami.jpl.nasa.gov>

Bill Steigerwald
NASA Goddard Space Flight Center, Greenbelt, Md. March 9, 2007

Lori Stiles
University of Arizona, Tuscon, AZ

Proposed Mission Will Return Sample from Near-Earth Object

A menacing lump of rock and dust in space called 10195 (1999 RQ36) would
barely be noticed except for two crucial facts: First, "It's a treasure
trove of organic material, so it holds clues to how Earth formed and life
got started," said Joseph Nuth of NASA's Goddard Space Flight Center,
Greenbelt, Md. Second, it regularly crosses Earth's orbit, so it might
impact us someday.

Nuth is Project Scientist for the proposed OSIRIS mission, which will
"return a pristine sample of the scientifically priceless asteroid RQ36 to
Earth for in-depth study," said University of Arizona Lunar and Planetary
Laboratory (LPL) Director Michael Drake, Principal Investigator for the
proposed mission. The mission will be the first to return a sample of an
asteroid to Earth. NASA Goddard is managing the project. Lockheed Martin is
building the flight system, the sampling mechanism, and the sample return
capsule. Lockheed Martin is also performing spacecraft operations.

The OSIRIS team recently won a $1.2 million award from NASA to develop a
more detailed engineering study of how the mission will accomplish its
scientific objectives. OSIRIS will launch in 2011, acquire a sample of RQ36
in 2013, and return it to Earth in 2017.

OSIRIS is both a mythological figure and an acronym. "O" stands for the
scientific theme, origins. "SI" is for spectral interpretation, or taking
images of the NEO at wavelengths that will reveal its composition. "RI," or
resource identification, is surveying the asteroid for such useful resources
as water and metals. "S" stands for security, learning how to predict the
detailed motion of Earth-approaching asteroids.

"OSIRIS of Egyptian mythology is the god of life and fertility, the god who
taught Egyptians agriculture," said Dante Lauretta, OSIRIS Deputy Principal
Investigator, also with the University of Arizona. "There's an analogy to
the proposed 21st century space mission. We're looking at the kind of object
that we think brought life to Earth; that is, objects that seeded Earth with
early biomolecules, the precursors of life."

Returning a sample to Earth will allow for a much more comprehensive study
of the NEO, according to the team. "The equipment in my lab is small, merely
desk-sized, but that's not easy to fly. Let alone the enormous synchrotrons,
which dwarf cars and are impossible to fly," said Jason Dworkin, also of
NASA Goddard, who is the Deputy Project Scientist and a Co-Investigator on
OSIRIS. "Furthermore, there are also a lot of steps to prepare a sample.
That would all have to be automated and work perfectly on a spacecraft."

"Also, you can't respond to surprises with the limited equipment on board a
spacecraft," added Nuth. "About thirty years ago, the Viking landers scooped
up a sample of Martian dirt and tested it for signs of microscopic life. The
results were contradictory, and ever since then, there's been a controversy
over whether there really was life or whether it was just some kind of
exotic chemical reaction. If instead we were able to return samples to
Earth, we could have tested the sample in other ways. And when technology
improves, we just take samples out and test with the latest equipment.
That's what we'll be able to do with the sample returned by OSIRIS."

OSIRIS samples will be available to the world-wide community, so people with
diverse skills and techniques can offer unique insights. "The Stardust
mission returned samples of comet Wild 2 with a total weight of just a tenth
of a milligram, but it is enough to be analyzed by researchers all over the
world," said Dworkin. "OSIRIS will return 150 grams -- about five ounces.
We'll take it apart almost atom by atom. It will keep a lot of people busy
for a long time."

The mission will also help to better track the orbits of asteroids that
might hit Earth by accurately measuring the "Yarkovsky effect" for the first
time. The Yarkovsky effect is a small push on an asteroid that happens when
the asteroid absorbs sunlight and emits heat. The small push adds up over
time, and it is uneven due to an asteroid's various surface materials,
wobble, and rotation. There's no sure way to predict an Earth-approaching
asteroid's orbit unless you can factor in how the Yarkovsky effect will
change that orbit, according to the team. "It's like trying to make a
complex, banking shot in a game of pool with someone shaking the table and
kicking the legs," said Nuth.

RQ36 is roughly 580 meters in diameter, or about two-fifths of a mile. It
orbits between about 83 million and 126 million miles from the sun, swinging
within about 280,000 miles of Earth orbit, or roughly 40,000 miles more
distant than the moon. The International Astronomical Union's Minor Planet
Center has officially classified RQ36 as a "potentially hazardous asteroid."

"It doesn't present any near-term hazard, but the small Yarkovsky push over
hundreds of orbits may eventually be enough to cause an 'oops'," said Nuth.

The OSIRIS proposal was among approximately two dozen submitted in response
to NASA's Discovery Program 2006 Announcement of Opportunity in April. NASA
also selected two other proposed new Discovery-class missions, and three
more Discovery-class proposals that would make use of existing NASA
spacecraft, for concept development funding. NASA may select one or more
investigations to continue into a development effort after detailed review
of the concept studies. Decisions about which mission concepts will proceed
to development are expected in late 2007.

IMAGE CAPTION:
[http://www.nasa.gov/centers/goddard/images/content/170769main_osiris_lgweb.jpg
(40KB)]
This is an artist's concept of the OSIRIS spacecraft taking a sample of
asteroid RQ36. Credit: NASA/U. of Arizona
Received on Tue 13 Mar 2007 12:11:45 PM PDT