papers

Publications (18)

astro-ph.EP2019

The trans-Neptunian object (84922) 2003 VS2 through stellar occultations

Gustavo Benedetti-Rossi, P. Santos-Sanz, J. L. Ortiz +50

We present results from three world-wide campaigns that resulted in the detections of two single-chord and one multi-chord stellar occultations by the Plutino object (84922) 2003~V…

astro-ph.EP2015

Pluto's atmosphere from stellar occultations in 2012 and 2013

A. Dias-Oliveira, B. Sicardy, E. Lellouch +42

We analyze two multi-chord stellar occultations by Pluto observed on July 18th, 2012 and May 4th, 2013, and monitored respectively from five and six sites. They provide a total of…

astro-ph.EP2009

A Giant Crater on 90 Antiope?

P. Descamps, F. Marchis, T. Michalowski +11

Mutual event observations between the two components of 90 Antiope were carried out in 2007-2008. The pole position was refined to lambda0 = 199.5+/-0.5 eg and beta0 = 39.8+/-5 deg…

astro-ph.EP2019

Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016

E. Meza, B. Sicardy, M. Assafin +167

Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by th…

astro-ph.EP2010

Formation of asteroid pairs by rotational fission

P. Pravec, D. Vokrouhlicky, D. Polishook +23

Asteroid pairs sharing similar heliocentric orbits were found recently. Backward integrations of their orbits indicated that they separated gently with low relative velocities, but…

astro-ph.EP2019

A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling technique

P. Bartczak, A. Kryszczyńska, G. Dudziński +12

We present a new non-convex model of the binary asteroid (809) Lundia. A SAGE (Shaping Asteroids with Genetic Evolution) method using disc-integrated photometry only was used for d…

astro-ph.EP2016

Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations

F. Marchis, J. E. Enriquez, J. P. Emery +13

Photometric lightcurves were also obtained for 14 of them during the Spitzer observations to provide the context of the observations and reliable estimates of their absolute magnit…

astro-ph.EP2021

Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020

B. E. Morgado, B. Sicardy, F. Braga-Ribas +78

The Centaur (10199) Chariklo has the first rings system discovered around a small object. It was first observed using stellar occultation in 2013. Stellar occultations allow the de…

astro-ph.EP2012

Analysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger - search for the YORP effect

J. Durech, D. Vokrouhlicky, A. R. Baransky +28

The spin state of small asteroids can change on a long timescale by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, the net torque that arises from anisotropically scatter…

astro-ph.EP2026

Constraining the size, shape, and albedo of the large Trans-Neptunian Object (28978) Ixion with multi-chord stellar occultations

Y. Kilic, F. Braga-Ribas, C. L. Pereira +81

Trans-Neptunian objects (TNOs) are among the most primitive remnants of the early Solar System, and constraining their sizes, shapes, albedos, and surface properties is essential f…

astro-ph.EP2010

Triplicity and Physical Characteristics of Asteroid (216) Kleopatra

Pascal Descamps, F. Marchis, J. Berthier +16

To take full advantage of the September 2008 opposition passage of the M-type asteroid (216) Kleopatra, we have used near-infrared adaptive optics (AO) imaging with the W.M. Keck I…

astro-ph.EP2023

Physical properties of Centaur (60558) 174P/Echeclus from stellar occultations

C. L. Pereira, F. Braga-Ribas, B. Sicardy +42

The Centaur (60558) Echeclus was discovered on March 03, 2000, orbiting between the orbits of Jupiter and Uranus. After exhibiting frequent outbursts, it also received a comet desi…

astro-ph.EP2017

The structure of Chariklo's rings from stellar occultations

D. Bérard, B. Sicardy, J. I. B. Camargo +79

Two narrow and dense rings (called C1R and C2R) were discovered around the Centaur object (10199) Chariklo during a stellar occultation observed on 2013 June 3. Following this disc…

astro-ph.EP2014

A ring system detected around the Centaur (10199) Chariklo

F. Braga-Ribas, B. Sicardy, J. L. Ortiz +61

Until now, rings have been detected in the Solar System exclusively around the four giant planets. Here we report the discovery of the first minor-body ring system around the Centa…

astro-ph2008

New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses

P. Descamps, F. Marchis, J. Pollock +16

In 2007, the M-type binary asteroid 22 Kalliope reached one of its annual equinoxes. As a consequence, the orbit plane of its small moon, Linus, was aligned closely to the Sun's li…

astro-ph.EP2019

Asteroid pairs: a complex picture

P. Pravec, P. Fatka, D. Vokrouhlický +45

We studied 93 asteroid pairs. We estimated times elapsed since separation of pair members that are between 7*10^3 and a few 10^6 yr. We derived the rotation periods for all the pri…

astro-ph.EP2014

The binary near-Earth asteroid (175706) 1996 FG3 - An observational constraint on its orbital evolution

P. Scheirich, P. Pravec, S. A. Jacobson +23

Using our photometric observations taken between 1996 and 2013 and other published data, we derived properties of the binary near-Earth asteroid (175706) 1996 FG3 including new mea…

astro-ph.EP2009

New insights on the binary asteroid 121 Hermione

P. Descamps, F. Marchis, J. Durech +29

We report on the results of a six-month photometric study of the main-belt binary C-type asteroid 121 Hermione, performed during its 2007 opposition. We took advantage of the rare…