Large size and slow rotation of the trans-Neptunian object (225088) 2007 OR10 discovered from Herschel and K2 observations [PDF]
We present the first comprehensive thermal and rotational analysis of the second most distant trans-Neptunian object (225088) 2007 OR10. We combined optical light curves provided by the Kepler space telescope -- K2 extended mission and thermal infrared ...
Kiss, Csaba +7 more
core +3 more sources
Generation of Highly Inclined Trans-Neptunian Objects by Planet Nine [PDF]
The trans-Neptunian region of the solar system exhibits an intricate dynamical structure, much of which can be explained by an instability-driven orbital history of the giant planets.
Batygin, Konstantin, Brown, Michael E.
core +2 more sources
Origin and Dynamical Evolution of Neptune Trojans - I: Formation and Planetary Migration [PDF]
We present the results of detailed dynamical simulations of the effect of the migration of the four giant planets on both the transport of pre-formed Neptune Trojans, and the capture of new Trojans from a trans-Neptunian disk.
B. W. Jones +48 more
core +3 more sources
Volatile evolution and atmospheres of Trans-Neptunian objects [PDF]
At 30-50 K, the temperatures typical for surfaces in the Kuiper Belt (e.g. Stern & Trafton 2008), only seven species have sublimation pressures higher than 1 nbar (Fray & Schmitt 2009): Ne, N$_2$, CO, Ar, O$_2$, CH$_4$, and Kr. Of these, N$_2$, CO, and CH$_4$ have been detected or inferred on the surfaces of Trans-Neptunian Objects (TNOs).
Young, Leslie A. +2 more
openaire +2 more sources
Light Curves of Trans-Neptunian Objects from the K2 Mission of the Kepler Space Telescope
The K2 mission of the Kepler Space Telescope allowed the observations of light curves of small solar system bodies throughout the whole solar system. In this paper, we present the results of a collection of K2 trans-Neptunian object observations between ...
Viktória Kecskeméthy +12 more
doaj +1 more source
The scattered trans-Neptunian object 1998 XY95 [PDF]
On 1998 December 12 a new trans-Neptunian object, 1998 XY95, was discovered as part of a deep search. Recent observations of this object have placed it amongst the class of objects known as the scattered trans-Neptunian objects (TNOs). A total of 39 CCD images of 1998 XY95 were taken over two nights, and these were used to search for a light curve, but
Collander-Brown, S.J. +4 more
openaire +1 more source
2008 OG19: a highly elongated Trans-Neptunian object [PDF]
Accepted in Monthly Notices of the Royal Astronomical Society; November 18 ...
Fernández Valenzuela, Estela del Mar +4 more
openaire +3 more sources
Pairs of Trans-Neptunian Objects with close orbits [PDF]
A search for pairs of dynamically correlated trans-Neptunian objects with semi-major axes of more than 30 au was performed. The Kholshevnikov metrics in the space of Keplerian orbits are used. Found 27 pairs with metrics less than 0.07 au1/2, 22 pairs in which one of the components is binary, for metrics less than 0.12 au1/2, and 11 pairs of binary ...
E. D. Kuznetsov +3 more
openaire +1 more source
Steeper Scattered Disks Buckle Faster
Disks of low-mass bodies scattered by giant planets to large semimajor axis and constant periapsis orbits are vulnerable to a buckling instability. This instability exponentially grows orbital inclinations, raises periapsis distances, and coherently ...
Alexander Zderic, Ann-Marie Madigan
doaj +1 more source
Neptune Trojans and Plutinos: colors, sizes, dynamics, and their possible collisions [PDF]
Neptune Trojans and Plutinos are two subpopulations of trans-Neptunian objects located in the 1:1 and the 3:2 mean motion resonances with Neptune, respectively, and therefore protected from close encounters with the planet.
A. C. M. Correia +49 more
core +2 more sources

