Abstract
The paper presents an analysis of the real change in brightness of comet 174P/Echeclus (60558 Echeclus), using the cryovolcanism mechanism. The relationship between the mass ejected during the outburst and the active surface during quiet sublimation is also presented. It has been shown that the mass ejected is one of the key parameters determining the change in the brightness of a comet. This assumption was also confirmed by many years of observations of comets during their outbursts.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
