ABSTRACT: There is a group of newly recognized asteroids in the main belt that are exhibiting cometary characteristics. We will call them Asteroidal Belt Comets or ABCs for short. The surprising property of these objects is that their orbits are entirely asteroidal while their behaviour is entirely cometary, with Tisserand invariants larger than 3.0, while all Jupiter family comets have Tisserand invariants smaller than 3.0. An analysis of their orbital and physical properties has resulted in the following conclusion. (1) We define the ‘detached group (DG)’ as those objects that exhibit cometary characteristics (sublimating water) and have aphelion distances Q < 4.5 au. The DG contains all the ABCs traditionally recognized, plus a few other...
In the Nice model, the late heavy bombardment (LHB) is related to an orbital instability o...
Observational data obtained primarily during 1988 are analyzed and synthesized to develop a comprehe...
Context. The mysterious solar system object 133P/(7968) Elst-Pizarro is dynamically asteroidal, yet...
The practical distinctions between asteroids and comets, viewed as products of accretion on either s...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
ABSTRACT: The secular light-curves (SLCs) of comets C/2011 L4 Panstarrs and C/2012 S1 ISON are plott...
Context. Dynamically, 133P/Elst-Pizarro and 176P/LINEAR are main belt asteroids, likely members of t...
Aims. We study the time an asteroid in a cometary orbit must wait to receive a collision producing a...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
Abstract. Asteroids and comets have been thought to be two separate kinds of objects in our solar sy...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
New regularities for short-perihelion comets are found. Distant nodes of cometary orbits of Kreutz f...
Cometary activity in main-belt asteroids probes the ice content of these objects and provides clues ...
We observed comet 322P/SOHO 1 (P/1999 R1) from the ground and with the Spitzer Space Telescope when ...
2009 MS9 is a trans-Neptunian object (TNO) whose perihelion brings it close to the distance where so...
In the Nice model, the late heavy bombardment (LHB) is related to an orbital instability o...
Observational data obtained primarily during 1988 are analyzed and synthesized to develop a comprehe...
Context. The mysterious solar system object 133P/(7968) Elst-Pizarro is dynamically asteroidal, yet...
The practical distinctions between asteroids and comets, viewed as products of accretion on either s...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
ABSTRACT: The secular light-curves (SLCs) of comets C/2011 L4 Panstarrs and C/2012 S1 ISON are plott...
Context. Dynamically, 133P/Elst-Pizarro and 176P/LINEAR are main belt asteroids, likely members of t...
Aims. We study the time an asteroid in a cometary orbit must wait to receive a collision producing a...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
Abstract. Asteroids and comets have been thought to be two separate kinds of objects in our solar sy...
Context. Determining whether asteroids in cometary orbits (ACOs) are dormant or extinct comets is re...
New regularities for short-perihelion comets are found. Distant nodes of cometary orbits of Kreutz f...
Cometary activity in main-belt asteroids probes the ice content of these objects and provides clues ...
We observed comet 322P/SOHO 1 (P/1999 R1) from the ground and with the Spitzer Space Telescope when ...
2009 MS9 is a trans-Neptunian object (TNO) whose perihelion brings it close to the distance where so...
In the Nice model, the late heavy bombardment (LHB) is related to an orbital instability o...
Observational data obtained primarily during 1988 are analyzed and synthesized to develop a comprehe...
Context. The mysterious solar system object 133P/(7968) Elst-Pizarro is dynamically asteroidal, yet...