activity
20092023
most citedColors and taxonomy of Centaurs and Trans-Neptunian Objects

86 citations · 648 across the 23 of their papers we have counts for

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Showing astro-ph.EPShow all

22 papers · 1 filter

astro-ph.EP2023★ 11 cited

Compositional properties of planet-crossing asteroids from astronomical surveys

A. V. Sergeyev, B. Carry, M. Marsset +8

Context. The study of planet-crossing asteroids is of both practical and fundamental importance. As they are closer than asteroids in the Main Belt, we have access to a smaller siz…

astro-ph.EP2023★ 7 cited

NEOROCKS project: surface properties of small near-Earth asteroids

T. Hromakina, M. Birlan, M. A. Barucci +11

We present new results of the observing program which is a part of the NEOROCKS project aimed to improve knowledge on physical properties of near-Earth Objects (NEOs) for planetary…

astro-ph.EP2019★ 12 cited

Long-term photometric monitoring of the dwarf planet (136472) Makemake

T. A. Hromakina, I. N. Belskaya, Yu. N. Krugly +17

We studied the rotational properties of the dwarf planet Makemake. The photometric observations were carried out at different telescopes between 2006 and 2017. Most of the measurem…

astro-ph.EP2018★ 10 cited

Basaltic material in the main belt: a tale of two (or more) parent bodies?

S. Ieva, E. Dotto, D. Lazzaro +5

The majority of basaltic objects in the main belt are dynamically connected to Vesta, the largest differentiated asteroid known. Others, due to their current orbital parameters, ca…

astro-ph.EP2018★ 17 cited

Photometric survey of 67 near-Earth objects

S. Ieva, E. Dotto, E. Mazzotta Epifani +9

The near-Earth object (NEO) population is a window into the original conditions of the protosolar nebula, and has the potential to provide a key pathway for the delivery of water a…

astro-ph.EP2018★ 79 cited

A spectroscopic survey of the small near-Earth asteroid population: peculiar taxonomic distribution and phase reddening

Davide Perna, Maria Antonietta Barucci, Marcello Fulchignoni +6

We present the results of the first-ever visible spectroscopic survey fully dedicated to the small (absolute magnitude H>20) near-Earth asteroid (NEA) population. Observations have…

astro-ph.EP2017★ 6 cited

Rotationally-resolved spectroscopy of Jupiter Trojans (624) Hektor and (911) Agamemnon

Davide Perna, Nicolas Bott, Tetiana Hromakina +3

We present the first-ever rotationally resolved spectroscopic investigation of (624) Hektor and (911) Agamemnon, the two largest Jupiter Trojans. The visible and near-infrared spec…

astro-ph.EP2017★ 3 cited

Photometric observations of nine Transneptunian objects and Centaurs

T. Hromakina, D. Perna, I. Belskaya +3

We present the results of photometric observations of six Transneptunian objects and three Centaurs, estimations of their rotational periods and corresponding amplitudes. For six o…

astro-ph.EP2017★ 14 cited

TNOs are Cool: a survey of the Transneptunian Region XII. Thermal light curves of Haumea, 2003 VS2 and 2003 AZ84 with Herschel Space Observatory-PACS

P. Santos-Sanz, E. Lellouch, O. Groussin +10

Time series observations of the dwarf planet Haumea and the Plutinos 2003VS2 and 2003AZ84 with Herschel/PACS are presented in this work. Thermal emission of these trans-Neptunian o…

astro-ph.EP2016★ 34 cited

Decimetre-scaled spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from OSIRIS observations

C. Feller, S. Fornasier, P. H. Hasselmann +43

We present the results of the photometric and spectrophotometric properties of the 67P/Churyumov-Gerasimenko nucleus derived with the OSIRIS instrument during the closest fly-by ov…

astro-ph.EP2016★ 9 cited

An investigation of the low-DeltaV near-Earth asteroids (341843) 2008 EV5 and (52381) 1993 HA. Two suitable targets for the ARM and MarcoPolo-M5 space missions

D. Perna, M. Popescu, F. Monteiro +3

The Asteroid Redirect Mission (ARM) under development by NASA is being planned to collect a multi-meter boulder from a near-Earth asteroid (NEA), and to bring it to the cis-lunar s…

astro-ph.EP2016★ 45 cited

Detection of exposed HO ice on the nucleus of comet 67P/Churyumov-Gerasimenko

M. A. Barucci, G. Filacchione, S. Fornasier +42

Since the orbital insertion of the Rosetta spacecraft, comet 67P/Churyumov-Gerasimenko (67P/C-G) has been mapped by OSIRIS camera and VIRTIS spectro-imager, producing a huge quanti…

astro-ph.EP2016★ 54 cited

Spectral variability on primitive asteroids of the Themis and Beagle families: space weathering effects or parent body heterogeneity?

S. Fornasier, C. Lantz, D. Perna +3

Themis is an old and statistically robust asteroid family populating the outer main belt, and resulting from a catastrophic collision that took place 2.51.0 Gyr ago. Within th…

astro-ph.EP2015★ 16 cited

Short-term variability on the surface of (1) Ceres. A changing amount of water ice?

D. Perna, Z. Kaňuchová, S. Ieva +5

Context: The dwarf planet (1) Ceres - next target of the NASA Dawn mission - is the largest body in the asteroid main belt; although several observations of this body have been per…

astro-ph.EP2014★ 18 cited

Non-gravitational Perturbations and Virtual Impactors: the case of asteroid 2009 FD

F. Spoto, A. Milani, D. Farnocchia +5

Asteroid 2009 FD could impact Earth between 2185 and 2196. The long term propagation to the possible impacts and the intervening planetary encounters make 2009 FD one of the most c…

astro-ph.EP2014★ 21 cited

Low delta-V near-Earth asteroids: A survey of suitable targets for space missions

S. Ieva, E. Dotto, D. Perna +7

In the last decades Near-Earth Objects (NEOs) have become very important targets to study, since they can give us clues to the formation, evolution and composition of the Solar Sys…

astro-ph.EP2011★ 33 cited

The spectrum of (136199) Eris between 350 and 2350 nm: Results with X-Shooter

A. Alvarez-Candal, N. Pinilla-Alonso, J. Licandro +7

X-Shooter is the first second-generation instrument for the ESO-VLT. It as a spectrograph covering the 300 - 2480 nm spectral range at once with a high resolving power. These prope…

astro-ph.EP2010★ 56 cited

Physical properties of ESA Rosetta target asteroid (21) Lutetia: Shape and flyby geometry

B. Carry, M. Kaasalainen, C. Leyrat +22

Aims. We determine the physical properties (spin state and shape) of asteroid (21) Lutetia, target of the ESA Rosetta mission, to help in preparing for observations during the flyb…

astro-ph.EP2010★ 27 cited

A Peculiar Family of Jupiter Trojans: the Eurybates

F. De Luise, E. Dotto, S. Fornasier +4

The Eurybates family is a compact core inside the Menelaus clan, located in the L4 swarm of Jupiter Trojans. Fornasier et al. (2007) found that this family exhibits a peculiar abun…

astro-ph.EP2010★ 20 cited

Inhomogeneities on the surface of 21 Lutetia, the asteroid target of the Rosetta mission

D. Perna, E. Dotto, M. Lazzarin +6

CONTEXT: In July 2010 the ESA spacecraft Rosetta will fly-by the main belt asteroid 21 Lutetia. Several observations of this asteroid have been so far performed, but its surface co…

astro-ph.EP2009★ 86 cited

Colors and taxonomy of Centaurs and Trans-Neptunian Objects

D. Perna, M. A. Barucci, S. Fornasier +6

The study of the surface properties of Centaurs and Trans-Neptunian Objects (TNOs) provides essential information about the early conditions and evolution of the outer Solar System…

astro-ph.EP2009★ 67 cited

Visible spectroscopy of the new ESO Large Program on trans-Neptunian objects and Centaurs: final results

S. Fornasier, M. A. Barucci, C. de Bergh +8

A second large programme (LP) for the physical studies of TNOs and Centaurs, started at ESO Cerro Paranal on October 2006 to obtain high-quality data, has recently been concluded.…