An out of this world asteroid – literally – has been observed for the first time ever with astronomers suggesting that the asteroid is a visitor to our Solar System and has arrived from interstellar space.
Using ESO’s Very Large Telescope in Chile and other observatories around the world, astronomers have been able to determine the shape of this unique object that is said to have traveled through space for millions of years before entering our Solar System. Astronomers have determined that the asteroid is a dark, reddish, highly-elongated rocky or high-metal-content object.
The asteroid was first spotted by the Pan-STARRS telescope in Hawai`i on October 19 when it picked up a faint point of light moving across the sky. Astronomers first believed it is a typical fast-moving small asteroid, but further observations allowed them to determine its orbit fairly accurately revealing that it has entered our Solar System from interstellar space and isn’t part of our Solar System unlike other asteroids and comets generally observed.
Although originally classified as a comet, observations from ESO and elsewhere revealed no signs of cometary activity after it passed closest to the Sun in September 2017. The object was reclassified as an interstellar asteroid and named 1I/2017 U1 (`Oumuamua).
“We had to act quickly,” explains team member Olivier Hainaut from ESO in Garching, Germany. “`Oumuamua had already passed its closest point to the Sun and was heading back into interstellar space.”
ESO’s Very Large Telescope was immediately called into action to measure the object’s orbit, brightness and colour more accurately than smaller telescopes could achieve. Speed was vital as `Oumuamua was rapidly fading as it headed away from the Sun and past the Earth’s orbit, on its way out of the solar system. There were more surprises to come.
Combining the images from the FORS instrument on the VLT using four different filters with those of other large telescopes, the team of astronomers led by Karen Meech (Institute for Astronomy, Hawai`i, USA) found that `Oumuamua varies dramatically in brightness by a factor of 10 as it spins on its axis every 7.3 hours.
Karen Meech explains the significance: “This unusually large variation in brightness means that the object is highly elongated: about ten times as long as it is wide, with a complex, convoluted shape. We also found that it has a dark red colour, similar to objects in the outer solar system, and confirmed that it is completely inert, without the faintest hint of dust around it.”
These properties suggest that `Oumuamua is dense, possibly rocky or with high metal content, lacks significant amounts of water or ice, and that its surface is now dark and reddened due to the effects of irradiation from cosmic rays over millions of years. It is estimated to be at least 400 metres long.
Preliminary orbital calculations suggested that the object had come from the approximate direction of the bright star Vega, in the northern constellation of Lyra. However, even travelling at a breakneck speed of about 95,000 kilometres/hour, it took so long for the interstellar object to make the journey to our solar system that Vega was not near that position when the asteroid was there about 300,000 years ago. `Oumuamua may well have been wandering through the Milky Way, unattached to any star system, for hundreds of millions of years before its chance encounter with the solar system.
Astronomers estimate that an interstellar asteroid similar to `Oumuamua passes through the inner solar system about once per year, but they are faint and hard to spot so have been missed until now. It is only recently that survey telescopes, such as Pan-STARRS, are powerful enough to have a chance to discover them.
“We are continuing to observe this unique object,” concludes Olivier Hainaut, “and we hope to more accurately pin down where it came from and where it is going next on its tour of the galaxy. And now that we have found the first interstellar rock, we are getting ready for the next ones!”
The new results appear in the journal Nature.