On the night of July 7, 2022, the Lowell Discovery Telescope near Flagstaff, Arizona captured this sequence in which the asteroid Didymos, located near the center of the screen, moves across the night sky. The sequence is sped up by about 900 times. Scientists used this and other observations from the July campaign to confirm Dimorphos’ orbit and anticipated location at the time of DART’s impact. Credits: Lowell Observatory/N. Moskovitz
Using some of the
world’s most powerful telescopes, the DART investigation team last month
completed a six-night observation campaign to confirm earlier calculations of
the orbit of Dimorphos—DART’s asteroid target—around its larger parent asteroid,
Didymos, confirming where the asteroid is expected to be located at the time of
impact. DART, which is the world’s first attempt to change the speed and path
of an asteroid’s motion in space, tests a method of asteroid deflection that
could prove useful if such a need arises in the future for planetary
defense.
“The measurements the team made in early 2021 were
critical for making sure that DART arrived at the right place and the right
time for its kinetic impact into Dimorphos,” said Andy Rivkin, the DART
investigation team co-lead at the Johns Hopkins University Applied Physics
Laboratory (APL) in Laurel, Maryland. “Confirming those measurements with new
observations shows us that we don’t need any course changes and we’re already
right on target.”
However, understanding the dynamics of
Dimorphos’ orbit is important for reasons beyond ensuring DART’s impact. If
DART succeeds in altering Dimorphos’ path, the moonlet will move closer toward
Didymos, shortening the time it takes to orbit it. Measuring that change is
straightforward, but scientists need to confirm that nothing other than the
impact is affecting the orbit. This includes subtle forces such as
radiation recoil from the asteroid’s Sun-warmed surface, which can gently push
on the asteroid and cause its orbit to change.
“The before-and-after nature of this
experiment requires exquisite knowledge of the asteroid system before we do
anything to it,” said Nick Moskovitz, an astronomer with Lowell Observatory in
Flagstaff, Arizona, and co-lead of the July observation campaign.
“We don’t want to, at the last minute, say, ‘Oh, here’s something we
hadn’t thought about or phenomena we hadn’t considered.’ We want to be sure
that any change we see is entirely due to what DART did.”
In late September to early October, around
the time of DART’s impact, Didymos and Dimorphos will make their closest
approach to Earth in recent years at approximately 6.7 million miles (10.8
million kilometers) away. Since March 2021 the Didymos system had been out of
range of most ground-based telescopes because of its distance from Earth, but
early this July the DART Investigation Team employed powerful telescopes in
Arizona and Chile — the Lowell Discovery Telescope at Lowell
Observatory, the Magellan Telescope at Las Campanas Observatory and the
Southern Astrophysical Research (SOAR) Telescope — to observe the
asteroid system and look for changes in its brightness. These changes, called
“mutual events,” occur when one of the asteroids passes in front of the other
because of Dimorphos’ orbit, blocking some of the light they
emit.
“It was a tricky time of year to get these
observations,” said Moskovitz. In the Northern Hemisphere, the nights are
short, and it is monsoon season in Arizona. In the Southern Hemisphere, the threat
of winter storms loomed. In fact, just after the observation campaign, a
snowstorm hit Chile, prompting evacuations from the mountain where SOAR is
located. The telescope was then shut down for close to ten days. “We asked for
six half-nights of observation with some expectation that about half of those
would be lost to weather, but we only lost one night. We got really lucky.”
In all, the team was able to extract from
the data the timing of 11 new mutual events. Studying those changes in
brightness enabled scientists to determine precisely how long it takes
Dimorphos to orbit the larger asteroid and thereby predict where Dimorphos will
be located at specific moments in time, including when DART makes impact. The
results were consistent with previous calculations.
“We really have high confidence now that
the asteroid system is well understood and we are set up to understand what
happens after impact,” Moskovitz said.
Not only did this observation campaign
enable the team to confirm Dimorphos’ orbital period and expected location at
time of impact, but it also allowed team members to refine the
process they will use to determine whether DART successfully changed
Dimorphos’s orbit post-impact, and by how much.
In October, the team will again use
ground-based telescopes around the world to look for mutual events and
calculate Dimorphos’ new orbit, expecting that the time it takes the smaller
asteroid to orbit Didymos will have shifted by several minutes. These
observations will also help constrain theories that scientists around the world
have put forward about Dimorphos’ orbit dynamics and the rotation of both
asteroids.
Johns Hopkins APL manages the DART mission for NASA's Planetary Defense Coordination Office as a project of the agency’s Planetary Missions Program Office. DART is the world's first planetary defense test mission, intentionally executing a kinetic impact into Dimorphos to slightly change its motion in space. While neither asteroid poses a threat to Earth, the DART mission will demonstrate that a spacecraft can autonomously navigate to a kinetic impact on a relatively small target asteroid and that this is a viable technique to deflect an asteroid on a collision course with Earth if one is ever discovered. DART will reach its target on Sept. 26, 2022.
For more information about the DART
mission, visit: https://www.nasa.gov/dartmission
Source: DART
Team Confirms Orbit of Targeted Asteroid | NASA
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