Is the interstellar asteroid really a comet?

The interstellar object Oumuamua was discovered back on October 19, 2017, but the puzzle of its true nature has taken months to unravel, and may never be fully solved.

Meaning "scout from the distant past" in Hawaiian, Oumuamua was found by astronomers working with the University of Hawaii's Pan-STARRS1 survey as it came close to Earth's orbit. But what is it: an asteroid or a comet? As soon as it was spotted, astronomers from around the world were on the case.

The first clue: its trajectory. Extensive follow-up observations by the Canada-France-Hawai?i Telescope (CFHT), the European Space Agency's (ESA) Optical Ground Station telescope in Tenerife, Canary Islands, and other telescopes around the world have helped pin it down.

Oumuamua was first spotted about a month after its closest approach to the Sun, which took it within the orbit of Mercury. Unlike any asteroid or comet observed before, this new object sped past the Sun, approaching from "above" the plabe of the planets on a highly inclined orbit, moving fast enough (70,800 miles per hour as of July 1, 2018) to escape the Sun's gravitational pull and eventually depart our Solar System.

Initially, astronomers assumed Oumuamua was a comet. Current understanding of planet formation predicts more interstellar comets than interstellar asteroids. However, astronomers did not see evidence of gas emission or a dusty environment in the observations. Without these hallmarks of cometary activity, it was classified as the first interstellar asteroid.

But the story has another surprising twist.

Following the initial discovery observations with Pan-STARRS, a team of astronomers, led by Marco Micheli of ESA's SSA-NEO Coordination Centre and Karen Meech of the University of Hawaii Institute for Astronomy, continued to make high precision measurements of the object and its position using many ground-based facilities like CFHT, as well as the Hubble Space Telescope. The final images were taken with Hubble in January, before the object became too faint to observe as it sped away on its outbound orbit.

Contrary to their expectations, the team found that the object was not following the anticipated trajectory if only the gravity of the Sun and the planets were determining its path. "Unexpectedly, we found that Oumuamua was not slowing down as much as it should have due to just gravitational forces," says Marco, lead author of the paper reporting the team's findings published in the journal Nature. What could be causing this curious behavior?

Rigorous analysis ruled out a range of possible influences, such as radiation pressure or thermal effects from the Sun, or interaction with the Sun's solar wind. Other, less likely scenarios, such as a collision with another body, or Oumuamua being two separate, loosely held-together objects, were also discarded.

Comets contain ices that sublimate, or turn directly from a solid to a gas, when warmed by the Sun. This process drags out dust from the comet's surface to create a fuzzy "atmosphere" and sometimes a tail. The release of gas pressure at different locations and times can have the effect of pushing the comet slightly off-course compared with the expected path if only gravitational forces were at play.

"Thanks to the high quality of the observations we were able to characterize the direction and magnitude of the non-gravitational perturbation, which behaves the same way as comet outgassing," says Davide Farnocchia of NASA's Jet Propulsion Laboratory.

The team has not detected any dusty material or chemical signatures that would typically characterize a comet, even in the deepest images from ESO''s Very Large Telescope, Hubble, and the Gemini South telescope. "Oumuamua is small - no more than a half a mile long - and it could have been releasing a small amount of relatively large dust for it to have escaped detection," said Meech.

"To really understand Oumuamua we would need to send a space probe to it. This is actually possible, but it would be very expensive and take a long time to get there, so it isn't practical this time. We just have to be ready for the next one."

"It was extremely surprising that Oumuamua first appeared as an asteroid, given that we expect interstellar comets should be far more abundant, so we have at least solved that particular puzzle," says Olivier Hainaut of the European Southern Observatory. "It is still a tiny and weird object that is not behaving like a typical comet, but our results certainly lean towards it being a comet and not an asteroid after all."

Because of its small size and faintness, current observations of Oumuamua do not provide all the information astronomers need to determine important aspects of the comet's surface. "When Oumuamua was discovered, the astronomy community gathered as much data as possible, but ultimately, the object was just not visible long enough to answer all our questions," says Ken Chambers from Pan-STARRS.

"With Pan-STARRS monitoring the skies, we hope to discover more Oumuamua-like objects in the future and begin to answer the really interesting questions about this class of objects."

Research paper

Related Links
University of Hawaii at Manoa
Asteroid and Comet Mission News, Science and Technology

Tweet

Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Monthly Supporter
$5+ Billed Monthly

paypal only

SpaceDaily Contributor
$5 Billed Once

credit card or paypal

Rosetta unravels formation of sunrise jets
Gottingen, Germany (SPX) May 24, 2018
The atmosphere of Rosetta's comet 67P/Churyumov-Gerasimenko is far from homogeneous. In addition to sudden outbursts of gas and dust, daily recurring phenomena at sunrise can be observed. In these, evaporating gas and entrained dust are concentrated to form jet-like structures. A new study, led by the Max Planck Institute for Solar System Research (MPS) in Germany and published in the journal Nature Astronomy, now identifies the rugged, duck-shaped structure of the comet as the main cause of these ... read more