Typically, asteroids — like the one depicted in this
artist’s concept — originate from the main asteroid belt between the orbits of
Mars and Jupiter, but a small population of near-Earth objects may also come
from the Moon’s surface after being ejected into space by an impact.
NASA/JPL-Caltech
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The near-Earth object was likely
ejected into space after an impact thousands of years ago. Now it could
contribute new insights to asteroid and lunar science.
The small near-Earth object 2024
PT5 captured the world’s attention last year after a NASA-funded telescope
discovered it lingering close to, but never orbiting, our planet for several
months. The asteroid, which is about 33 feet (10 meters) wide, does not pose a
hazard to Earth, but its orbit around the Sun closely matches that of our
planet, hinting that it may have originated nearby.
As described in a study published Jan. 14 in the Astrophysical Journal Letters, researchers have
collected further evidence of 2024 PT5 being of local origin: It appears to be
composed of rock broken off from the Moon’s surface and ejected into space
after a large impact.
“We had a general idea that this
asteroid may have come from the Moon, but the smoking gun was when we found out
that it was rich in silicate minerals — not the kind that are seen on asteroids
but those that have been found in lunar rock samples,” said Teddy Kareta, an
astronomer at Lowell Observatory in Arizona, who led the research. “It looks
like it hasn’t been in space for very long, maybe just a few thousand years or
so, as there’s a lack of space weathering that would have caused its spectrum
to redden.”
The asteroid was first detected on Aug. 7, 2024, by the NASA-funded Sutherland, South Africa,
telescope of the University of Hawai’i’s Asteroid Terrestrial-impact Last Alert
System (ATLAS). Kareta’s team then used observations from the Lowell Discovery
Telescope and the NASA Infrared Telescope Facility (IRTF) at the Mauna Kea Observatory in Hawai’i to show that
the spectrum of reflected sunlight from the small object’s surface didn’t match
that of any known asteroid type; instead, the reflected light more closely
matched rock from the Moon.
Not (Old)
Rocket Science
A second clue came from observing
how the object moves. Along with asteroids, Space Age debris, such as old
rockets from historic launches, can also be found in Earth-like orbits.
The difference in their orbits has to do with how each type responds to solar radiation pressure, which comes from the momentum of photons — quantum particles of light from the Sun — exerting a tiny force when they hit a solid object in space. This momentum exchange from many photons over time can push an object around ever so slightly, speeding it up or slowing it down. While a human-made object, like a hollow rocket booster, will move like an empty tin can in the wind, a natural object, such as an asteroid, will be much less affected.
Researchers studying asteroid 2024 PT5 have plotted
its looping motion on two graphs. To a trained eye, they show that the object
never gets captured by Earth’s gravity but, instead, lingers nearby before
continuing its orbit around the Sun.
NASA/JPL-Caltech
To rule out 2024 PT5 being space junk, scientists at NASA’s Center for Near
Earth Object Studies (CNEOS), which is managed by the agency’s Jet Propulsion
Laboratory in Southern California, analyzed its motion. Their precise
calculations of the object’s motion under the force of gravity ultimately
enabled them to search for additional motion caused by solar radiation
pressure. In this case, the effects were found to be too small for the object
to be artificial, proving 2024 PT5 is most likely of natural origin.
“Space debris and space rocks move
slightly differently in space,” said Oscar Fuentes-Muñoz, a study coauthor and
NASA postdoctoral fellow at JPL working with the CNEOS team. “Human-made debris
is usually relatively light and gets pushed around by the pressure of sunlight.
That 2024 PT5 doesn’t move this way indicates it is much denser than space
debris.”
Asteroid Lunar
Studies
The discovery of 2024 PT5 doubles
the number of known asteroids thought to originate from the Moon.
Asteroid 469219 Kamo’oalewa was found in 2016 with an Earth-like orbit around the Sun, indicating
that it may also have been ejected from the lunar surface after a large impact.
As telescopes become more sensitive to smaller asteroids, more potential Moon
boulders will be discovered, creating an exciting opportunity not only for
scientists studying a rare population of asteroids, but also for scientists
studying the Moon.
If a lunar asteroid can be directly
linked to a specific impact crater on the Moon, studying it could lend insights
into cratering processes on the pockmarked lunar surface. Also, material from
deep below the lunar surface — in the form of asteroids passing close to Earth
— may be accessible to future scientists to study.
“This is a story about the Moon as
told by asteroid scientists,” said Kareta. “It’s a rare situation where we’ve
gone out to study an asteroid but then strayed into new territory in terms of
the questions we can ask of 2024 PT5.”
The ATLAS, IRTF, and CNEOS projects are funded by NASA’s planetary defense program, which is managed by the Planetary Defense Coordination Office at NASA Headquarters in Washington.
By: Jet Propulsion Laboratory
Source: Study Finds Earth’s Small Asteroid Visitor Likely Chunk of Moon Rock - NASA
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