Spitzer Observations of Interstellar Object ‘Oumuamua

Spitzer Observations of Interstellar Object 1I 'Oumuamua

An artist’s rendering of ‘Oumuamua, a visitor from outside the solar system. Astronomers used the IRAC camera on the Spitzer Space Telescope to set a limit on the infrared emission from ‘Oumuamua and thus to estimate its size. Credit: Joy Pollard / Gemini Observatory / AURA / NSF

One year ago this week astronomers discovered an unusual object moving through space not too far from the Earth’s orbit. In just a few days they realized it could not be a normal asteroid or comet – its path showed that it was not gravitationally bound to the solar system. It was, therefore, the first interstellar body ever discovered in our solar system that originated from outside it. It was given the Hawaiian name ‘Oumuamua, “scout.”

Astronomers have long thought that comets and asteroids exist in other planetary systems – perhaps ‘Oumuamua came from one of them. Most current models of our own Solar System suggest that such small bodies are leftovers from the era of planet formation, and other planetary systems should also have produced comets and asteroids. Studying them would offer powerful insights into the similarities and differences in planetary system formation. So far, however, it has been impossible: the presumed large populations of comets and asteroids found in exoplanetary circumstellar disks are far away and their individual members are faint and spatially unresolved.

‘Oumuamua might therefore be a rare scientific resource, and it became the subject of an intense, though brief, observing campaign – brief because it was so fast moving that it quickly became too distant and faint to detect. Nevertheless, the observations that were completed found that it was reddish in color, with no apparent spectral features and no signs of gas or dust. All these suggest it might be something like a primitive (“D-type”) asteroid, although in truth there is no good analog known in our solar system. Most remarkable of all, as it rotated its variable light curve revealed that it has a very elongated shape: six times longer than it is wide.

The IRAC camera on the Spitzer Space Telescope is currently about 155 million miles from Earth, and had a very different viewing angle toward ‘Oumuamua than did Earth-bound telescopes. CfA astronomers Joe Hora, Howard Smith and Giovanni Fazio, together with their long-standing team of Near Earth Object scientists and other colleagues, pointed IRAC at the spot in the sky where predictions placed ‘Oumuamua (because it is not bound to the Solar system and is so fast moving, ‘Oumuamua’s path in the sky was comparatively difficult to calculate).

After thirty hours of staring – a relatively long time – the object was not detected, and subsequent orbital analyses confirmed that the camera was pointed correctly towards it. The limit to its emission, however, was so low that it enabled the team to constrain some of its physical properties. The lack of an infrared signal, for example, suggests it has no gas or dust, species that would be expected if it were a cometary-like body.

The scientists also calculate that, depending on its exact composition and reflectivity, ‘Oumuamua is at least 240 meters (and maybe as much as one kilometer) in its longest dimension (for Star Trek aficionados, some fans estimate the length of the Enterprise to be 725 meters). The object has now moved too far for any of our telescopes to see it, and so although it will remain an interstellar mystery, it reminds us yet again that our cosmic neighborhood is full of surprises.

Publication: “Spitzer Observations of Interstellar Object 1I/’Oumuamua,” David E. Trilling, Michael Mommert, Joseph L. Hora, Davide Farnocchia, Paul Chodas, Jon Giorgini, Howard A. Smith, Sean Carey, Carey M. Lisse, Michael Werner, Andrew McNeill, Steven R. Chesley, Joshua P. Emery, Giovanni Fazio, Yanga R. Fernandez, Alan Harris, Massimo Marengo, Michael Mueller, Alissa Roegge, Nathan Smith, H. A. Weaver, Karen Meech, and Marco Micheli, AJ (in press) 2018.


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  • If my theory about dark matter having a liquid and a gaseous state is correct it would explain the acceleration of Oumuamua as the zero g spot at the center of the asteroid would be offset to the sunward side of the asteroid. When spritzer was looking for it it was well off the plane of the solar system so there would have been much less dark matter to phase transition and release heat, whereas on the way out of the solar system it was following fairly close to the plane. Would the James Webb telescope be able to see if it has gained any temperature. Or maybe watch for incoming asteroids along the plane where the temperature is higher than expected.

Megan Watzke, Harvard-Smithsonian Center for Astrophysics

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