Zobrazeno 1 - 10
of 911
pro vyhledávání: '"Transneptunian objects"'
Autor:
Kecskeméthy, Viktória, Kiss, Csaba, Szakáts, Róbert, Pál, András, Szabó, Gyula M., Molnár, László, Sárneczky, Krisztián, Vinkó, József, Szabó, Róbert, Marton, Gábor, Farkas-Takács, Anikó, Kalup, Csilla E., Kiss, László L.
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 transneptunian object observations, betwe
Externí odkaz:
http://arxiv.org/abs/2210.06571
There is a complex inclination structure present in the transneptunian object (TNO) orbital distribution in the main classical belt region (between orbital semimajor axes of 39 and 48 au). The long-term gravitational effects of the giant planets make
Externí odkaz:
http://arxiv.org/abs/2202.09045
In terms of scientific output, the best way to study solar system bodies is sending spacecraft to make in-situ measurements or to observe at close distance. Probably, the second best means to learn about important physical properties of solar system
Externí odkaz:
http://arxiv.org/abs/1905.04335
We present the results of photometric observations of six Transneptunian objects and three Centaurs, estimations of their rotational periods and corresponding amplitudes. For six of them we present also lower limits of density values. All observation
Externí odkaz:
http://arxiv.org/abs/1712.04284
The classical disturbing function of the three-body problem is based on an expansion of the gravitational interaction in the vicinity of nearly coplanar orbits. Consequently, it is not suitable for the identification and study of resonances of the Ce
Externí odkaz:
http://arxiv.org/abs/1707.02431
Autor:
Desmars, J., Camargo, J. I. B., Braga-Ribas, F., Vieira-Martins, R., Assafin, M., Vachier, F., Colas, F., Ortiz, J. L., Duffard, R., Morales, N., Sicardy, B., Gomes-Júnior, A. R., Benedetti-Rossi, G.
Publikováno v:
A&A 584, A96 (2015)
The prediction of stellar occultations by Transneptunian objects and Centaurs is a difficult challenge that requires accuracy both in the occulted star position as for the object ephemeris. Until now, the most used method of prediction involving tens
Externí odkaz:
http://arxiv.org/abs/1509.08674
Autor:
Lacerda, Pedro, Fornasier, Sonia, Lellouch, Emmanuel, Kiss, Csaba, Vilenius, Esa, Santos-Sanz, Pablo, Rengel, Miriam, Mueller, Thomas, Stansberry, John, Duffard, Rene, Delsanti, Audrey, Guilbert-Lepoutre, Aurelie
We analyze albedo data obtained using the Herschel Space Observatory that reveal the existence of two distinct types of surface among midsized transneptunian objects. A color-albedo diagram shows two large clusters of objects, one redder and higher a
Externí odkaz:
http://arxiv.org/abs/1406.1420
Autor:
Benecchi, Susan D., Sheppard, Scott S.
We present observations of 32 primarily bright, newly discovered Transneptunian objects observable from the Southern Hemisphere during 39 nights of observation with the 2.5-m telescope at Las Campanas Observatory. Our dataset includes objects in all
Externí odkaz:
http://arxiv.org/abs/1301.5791
Autor:
Kenyon, Scott J., Bromley, Benjamin C.
We investigate whether coagulation models of planet formation can explain the observed size distributions of transneptunian objects (TNOs). Analyzing published and new calculations, we demonstrate robust relations between the size of the largest obje
Externí odkaz:
http://arxiv.org/abs/1201.4395
We present optical colors of 72 transneptunian objects (TNOs), and infrared colors of 80 TNOs obtained with the WFPC2 and NICMOS instruments, respectively, on the Hubble Space Telescope (HST). Both optical and infrared colors are available for 32 obj
Externí odkaz:
http://arxiv.org/abs/1103.2175