Evidence that 1I/2017 U1 (`Oumuamua) was composed of molecular hydrogen ice
2020
Online
report
Zugriff:
`Oumuamua (I1 2017) was the first macroscopic ($l\sim100\,{\rm m}$) body observed to traverse the inner solar system on an unbound hyperbolic orbit. Its light curve displayed strong periodic variation, and it showed no hint of a coma or emission from molecular outgassing. Astrometric measurements indicate that 'Oumuamua experienced non-gravitational acceleration on its outbound trajectory, but energy balance arguments indicate this acceleration is inconsistent with a water ice sublimation-driven jet of the type exhibited by solar system comets. We show that all of `Oumaumua's observed properties can be explained if it contained a significant fraction of molecular hydrogen (H$_{2}$) ice. H$_{2}$ sublimation at a rate proportional to the incident solar flux generates a surface-covering jet that reproduces the observed acceleration. Mass wasting from sublimation leads to monotonic increase in the body axis ratio, explaining `Oumuamua's shape. Back-tracing `Oumuamua's trajectory through the Solar System permits calculation of its mass and aspect ratio prior to encountering the Sun. We show that H$_{2}$-rich bodies plausibly form in the coldest dense cores of Giant Molecular Clouds, where number densities are of order $n\sim10^5$, and temperatures approach the $T=3\,{\rm K}$ background. Post-formation exposure to galactic cosmic rays implies a $\tau \sim 100$ Myr age, explaining the kinematics of `Oumuamua's inbound trajectory.
Comment: Accepted for publication in ApJL, 8 pages, 2 figures. All software is available at https://github.com/DSeligman/Oumuamua_Hydrogen
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Evidence that 1I/2017 U1 (`Oumuamua) was composed of molecular hydrogen ice
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Autor/in / Beteiligte Person: | Seligman, Darryl ; Laughlin, Gregory |
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Veröffentlichung: | 2020 |
Medientyp: | report |
DOI: | 10.3847/2041-8213/ab963f |
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