Occurrence Rates of Exosatellites Orbiting 3-30M$_{\rm Jup}$ Hosts from 44 Spitzer Light Curves
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2024
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| _version_ | 1866909201154965504 |
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| author | Limbach, Mary Anne Vos, Johanna M. Vanderburg, Andrew Dai, Fei |
| author_facet | Limbach, Mary Anne Vos, Johanna M. Vanderburg, Andrew Dai, Fei |
| contents | We conduct a comprehensive search for transiting exomoons and exosatellites within 44 archival Spitzer light curves of 32 substellar worlds with estimated masses ranging between 3-30M$_{\rm Jup}$. This sample's median host mass is 16M$_{\rm Jup}$, inclusive of 14 planetary-mass objects, among which one is a wide-orbit exoplanet. We search the light curves for exosatellite signatures and implement a transit injection-recovery test, illustrating our survey's capability to detect $>$0.7R$_{\oplus}$ exosatellites. Our findings reveal no substantial ($>$5$σ$) evidence for individual transit events. However, an unusual fraction of light curves favor the transit model at the 2-3$σ$ significance level, with fitted transit depths consistent with terrestrial-sized (0.7-1.6R$_{\oplus}$) bodies. Comparatively, fewer than 2.2% of randomly generated normal distributions from an equivalent sample size exhibit a similar prevalence of outliers. Should one or two of these outliers represent a real exosatellite transit, it would imply an occurrence rate of $η= 0.61^{+0.49}_{-0.34}$ short-period terrestrial exosatellites per system, consistent with the known occurrences rates for both solar system moons and mid M-dwarf exoplanets. We explore alternative astrophysical interpretations for these outliers, underscoring that transits are not the only plausible explanation. For orbital periods $<$0.8 days, the typical duration of the light curves, we constrain the occurrence rate of sub-Neptunes to $η<$0.35 (95% confidence) and, if none of the detected outlier signals are real, the occurrence rate of terrestrial ($\sim$Earth-sized) exosatellites to $η<$0.51 (95% confidence). Forthcoming JWST observations of substellar light curves will enable detection of sub-Io-sized exosatellites, allowing for much stronger constraints on this exosatellite population. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2405_08116 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Occurrence Rates of Exosatellites Orbiting 3-30M$_{\rm Jup}$ Hosts from 44 Spitzer Light Curves Limbach, Mary Anne Vos, Johanna M. Vanderburg, Andrew Dai, Fei Earth and Planetary Astrophysics We conduct a comprehensive search for transiting exomoons and exosatellites within 44 archival Spitzer light curves of 32 substellar worlds with estimated masses ranging between 3-30M$_{\rm Jup}$. This sample's median host mass is 16M$_{\rm Jup}$, inclusive of 14 planetary-mass objects, among which one is a wide-orbit exoplanet. We search the light curves for exosatellite signatures and implement a transit injection-recovery test, illustrating our survey's capability to detect $>$0.7R$_{\oplus}$ exosatellites. Our findings reveal no substantial ($>$5$σ$) evidence for individual transit events. However, an unusual fraction of light curves favor the transit model at the 2-3$σ$ significance level, with fitted transit depths consistent with terrestrial-sized (0.7-1.6R$_{\oplus}$) bodies. Comparatively, fewer than 2.2% of randomly generated normal distributions from an equivalent sample size exhibit a similar prevalence of outliers. Should one or two of these outliers represent a real exosatellite transit, it would imply an occurrence rate of $η= 0.61^{+0.49}_{-0.34}$ short-period terrestrial exosatellites per system, consistent with the known occurrences rates for both solar system moons and mid M-dwarf exoplanets. We explore alternative astrophysical interpretations for these outliers, underscoring that transits are not the only plausible explanation. For orbital periods $<$0.8 days, the typical duration of the light curves, we constrain the occurrence rate of sub-Neptunes to $η<$0.35 (95% confidence) and, if none of the detected outlier signals are real, the occurrence rate of terrestrial ($\sim$Earth-sized) exosatellites to $η<$0.51 (95% confidence). Forthcoming JWST observations of substellar light curves will enable detection of sub-Io-sized exosatellites, allowing for much stronger constraints on this exosatellite population. |
| title | Occurrence Rates of Exosatellites Orbiting 3-30M$_{\rm Jup}$ Hosts from 44 Spitzer Light Curves |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2405.08116 |