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The process is akin to making a super-thin snake from a ball of Play-Doh. As the Play-Doh gets progressively thinner, smaller chunks start to shred off, with each of the bits still retaining their elongated shape.
Only in the vaguest of terms, finding stars it might have come from, or have influenced its path through space. The Sun is now another one of those pinball bumpers.
Any ideas as to where and how far this interstellar interloper travelled?
We use its newly determined non-Keplerian trajectory together with the reconstructed Galactic orbits of 7 million stars from Gaia DR2 to identify past close encounters. Such an "encounter" could reveal the home system from which 'Oumuamua was ejected. The closest encounter, at 0.60pc (0.53-0.67pc, 90% confidence interval), was with the M2.5 dwarf HIP 3757 at a relative velocity of 24.7km/s, 1Myr ago. A more distant encounter (1.6pc) but with a lower encounter (ejection) velocity of 10.7km/s was with the G5 dwarf HD 292249, 3.8Myr ago. Two more stars have encounter distances and velocities intermediate to these.
In a January 2019 study published in the International Journal of Astrobiology, Loeb and a Harvard undergraduate student Amir Siraj suggest that Earth-grazing comets and interstellar objects could have snagged microbes from high in our atmosphere and then carried them out into the Milky Way. Their estimates predict this could have already happened many times, depending on how high up life exists on our planet. "We found that there could be thousands, if not tens of thousands, that could pass through the Earth's atmosphere, collect microbes, and then get kicked to another solar system," Loeb says.
I remember reading about how it was unusually reflective.
Reflectivity of the surface of ‘Oumuamua The surface reflectivity of ‘Oumuamua is consistent with D-type asteroids¹⁰ and comets.
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originally posted by: Phage
a reply to: MissSmartypants
I remember reading about how it was unusually reflective.
No. The opposite, actually. Pretty typical.
Reflectivity of the surface of ‘Oumuamua The surface reflectivity of ‘Oumuamua is consistent with D-type asteroids¹⁰ and comets.
www.researchgate.net...
‘Oumuamua didn’t show signatures of ice or minerals found in rock, which means it’s neither icy nor rocky, at least not exactly. But it did show signs of carbon compounds. Fitzsimmons said previous studies have revealed that when carbon-rich, comet-like objects are exposed to the radiation that would be found in interstellar space, the material forms a crust that acts as insulation. If ‘Oumuamua has ice, as a comet would, it may be hiding beneath a mantle half a meter thick, formed after hundreds of millions—perhaps even billions—of years of bombardment by high-energy particles.
If there's any ice there, sounds like it's underneath the surface, not on top of it.
It's from an article on NASA.gov from Nov.14 2018 entitled "NASA Learns More About Interstellar Visitor Oumuanua".
originally posted by: Phage
a reply to: MissSmartypants
Passing the Sun gave it a coating of ice? That's interesting.
I don't suppose you have a link?
iopscience.iop.org...
Unfortunately, we do not have pre-perihelion observations to compare to these post-perihelion observations to test the hypothesis that 'Oumuamua brightened during its perihelion passage.