[meteorite-list] Versatile Instrument to Scout for Near-Earth Asteroids, Kuiper Belt Objects

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Fri, 4 Mar 2016 12:06:08 -0800 (PST)
Message-ID: <201603042006.u24K68kD001316_at_zagami.jpl.nasa.gov>

http://www.jpl.nasa.gov/news/news.php?feature=5702

Versatile Instrument to Scout for Kuiper Belt Objects
Jet Propulsion Laboratory
March 3, 2016

At the Palomar Observatory near San Diego, astronomers are busy tinkering
with a high-tech instrument that could discover a variety of objects both
far from Earth and closer to home.

The Caltech HIgh-speed Multi-color camERA (CHIMERA) system is looking
for objects in the Kuiper Belt, the band of icy bodies beyond the orbit
of Neptune that includes Pluto. It can also detect near-Earth asteroids
and exotic forms of stars. Scientists at NASA's Jet Propulsion Laboratory
and the California Institute of Technology, both in Pasadena, are collaborating
on this instrument.

"The Kuiper Belt is a pristine remnant of the formation of our solar system,"
said Gregg Hallinan, CHIMERA principal investigator at Caltech. "By studying
it, we can learn a large amount about how our solar system formed and
how it's continuing to evolve."

The wide-field telescope camera system allows scientists to monitor thousands
of stars simultaneously to see if a Kuiper Belt object passes in front
of any of them. Such an object would diminish a star's light for only
one-tenth of a second while traveling by, meaning a camera has to be fast
in order to capture it.

"Each of CHIMERA's cameras will be taking 40 frames per second, allowing
us to measure the distinct diffraction pattern in the wavelengths of light
to which they are sensitive," said Leon Harding, CHIMERA instrument scientist
at JPL. "This high-speed imaging technique will enable us to find new
Kuiper Belt objects far less massive in size than any other ground-based
survey to date."

Hallinan's CHIMERA team at Caltech and JPL published a paper led by Harding
describing the instrument this week in the Monthly Notices of the Royal
Astronomical Society.

Astronomers are particularly interested in finding Kuiper Belt objects
smaller than 0.6 miles (1 kilometer) in diameter. Since so few such objects
have ever been found, scientists want to figure out how common they are,
what they are made of and how they collide with other objects. The CHIMERA
astronomers estimate that in the first 100 hours of CHIMERA data, they
could find dozens of these small, distant objects.

Another scientific focus for CHIMERA is near-Earth asteroids, which the
instrument can detect even if they are only about 30 feet (10 meters)
across. Mike Shao of JPL, who leads the CHIMERA group's near-Earth asteroid
research effort, predicts that by using CHIMERA on the Hale telescope
at Palomar, they could find several near-Earth objects per night of telescope
observation.

Transient or pulsing objects such as binary star systems, pulsing white
dwarfs and brown dwarfs can also be seen with CHIMERA.

"What makes CHIMERA unique is that it does high-speed, wide-field, multicolor
imaging from the ground, and can be used for a wide variety of scientific
purposes," Hallinan said. "It's the most sensitive instrument of its kind."

CHIMERA uses detectors called electron multiplying charged-coupled devices
(EMCCDs), making for an extremely high-sensitivity, low-noise camera system.
One of the EMCCDs picks up near-infrared light, while the other picks
up green and blue wavelengths, and the combination allows for a robust
system of scanning perturbations in starlight. The detectors are capable
of running at minus 148 degrees Fahrenheit (minus 100 degrees Celsius)
in order to avoid noise when imaging fast objects.

"Not only can we image over a wide field, but in other modes we can also
image objects rotating hundreds of times per second," Harding said.

One of the objects the CHIMERA team used in testing the instrument's imaging
and timing abilities was the Crab Pulsar. This pulsar is the end result
of a star whose mass collapsed at the end of its life. It weighs as much
as our sun, but spins 32 times per second. The instrument focused on the
pulsar for a 300-second exposure to produce a color image.

"Our camera can image the entire field of view at 40 frames per second,"
Hallinan said. "We zoomed in on the pulsar and imaged it very fast, then
imaged the rest of the scene slowly to create an aesthetically-pleasing
image."

Highlighting CHIMERA's versatility, the instrument also imaged the globular
cluster M22, located in the constellation Sagittarius toward the busy
center of our galaxy. A single 25-millisecond image captured more than
1,000 stars. The team will be observing M22, and other fields like it,
for 50 nights over three years, to look for signatures of Kuiper Belt
objects.

Caltech manages JPL for NASA.


Media Contact

Elizabeth Landau
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6425
Elizabeth.Landau at jpl.nasa.gov

2016-059
Received on Fri 04 Mar 2016 03:06:08 PM PST