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Activity of (2060) Chiron possibly caused by impacts?
|Authors:||Cikota, Stefan; Fernández Valenzuela, Estela del Mar; Ortiz, José Luis ; Morales, Nicolás ; Duffard, René D. ; Aceituno, Jesús; Cikota, Aleksandar; Santos Sanz, Pablo|
Asteroids: individual: (2060) Chiron
planets and satellites: rings
|Publisher:||Oxford University Press|
|Citation:||Monthly Notices of the Royal Astronomical Society 475(2): 2512-2518 (2018)|
|Abstract:||The centaur 95P/(2060) Chiron is showing comet-like activity since its discovery, but the mass-loss mechanisms triggering its activity remained unexplained. Although the collision rates in the centaur region are expected to be very low, and impacts are thought not to be responsible for the mass-loss, since the recent indications that Chiron might possess a ring similar to Chariklo's, and assuming that there is debris orbiting around, the impact triggered mass-loss mechanism should not be excluded as a possible cause of its activity. From time series observations collected on Calar Alto Observatory in Spain between 2014 and 2016, we found that the photometric scatter in Chiron's data is larger than a control star's scatter, indicating a possible microactivity, possibly caused by debris falling back to Chiron's surface and lifting small clouds of material. We also present rotational light curves, and measurements of Chiron's absolute magnitudes, which are consistent with the models supporting the presumption that Chiron possesses rings. By co-adding the images acquired in 2015, we have detected an similar to 5 arcsec long tail, showing a surface brightness of 25.3 mag(V) arcsec(-2).© The Author 2018. Published by Oxford University Press on behalf of The Royal Astronomical Society.|
|Publisher version (URL):||http://dx.doi.org/10.1093/mnras/stx3352|
|Appears in Collections:||(IAA) Artículos|
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