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相关论文: Trans-Neptunian objects and Centaurs at thermal wa…

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Mid-IR albedo values of Neptune are derived from Spitzer Space Telescope measurements reported by Stauffer et al. (2016). The method of this derivation is described and the results indicate that the geometric albedo was about 1% or less at…

地球与行星天体物理 · 物理学 2018-03-12 Anthony Mallama , Liming Li

Context: Trans-Neptunian objects are distant bodies that retain valuable information about the origin and evolution of the Solar System. Many of these objects constitute binary systems. Studying binaries allows us to further characterise…

地球与行星天体物理 · 物理学 2026-05-22 J. M. Gómez-Limón , R. Leiva , J. L. Ortiz , P. Santos-Sanz , M. Kretlow , Y. Kilic , J. L. Rizos , A. Álvarez-Candal , T. G. Müller

We have measured the mid-infrared thermal continua from two Centaurs, inactive (8405) Asbolus and active 95P=(2060) Chiron, and have constrained their geometric albedos, p, and effective radii, R, with the Standard Thermal Model for slow…

天体物理学 · 物理学 2009-11-07 Y. R. Fernandez , D. C. Jewitt , S. S. Sheppard

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,…

地球与行星天体物理 · 物理学 2020-03-18 Leslie A. Young , Felipe Braga-Ribas , Robert E. Johnson

Trans-Neptunian objects (TNOs) in the outer Solar System are predominantly small, icy worlds long presumed to be atmosphereless except for the largest bodies. Until now, Pluto has been unique among TNOs in exhibiting a substantial…

地球与行星天体物理 · 物理学 2026-05-05 Ko Arimatsu , Fumi Yoshida , Tsutomu Hayamizu , Satoshi Takita , Katsumasa Hosoi , Takafumi Ootsubo , Jun-ichi Watanabe

The scattering trans-Neptunian Objects (TNOs) can be measured to smaller sizes than any other distant small-body population. We use the largest sample yet obtained, 68 discoveries, primarily by the Outer Solar System Origins Survey (OSSOS),…

Haumea is one of the most interesting and intriguing transneptunian objects (TNOs). It is a large, bright, fast rotator, and its spectrum indicates nearly pure water ice on the surface. It has at least two satellites and a dynamically…

地球与行星天体物理 · 物理学 2016-06-01 Audrey Thirouin , Scott S. Sheppard , Keith S. Noll , Nicholas A. Moskovitz , Jose-Luis Ortiz , Alain Doressoundiram

We present new optical reflectance spectra of three potentially silicate-rich trans-Neptunian Objects (TNOs). These spectra were obtained with the aim of confirming past hints and detections of 0.7 micron absorption features associated with…

地球与行星天体物理 · 物理学 2024-01-22 Tom Seccull , Wesley C. Fraser , Dominik A. Kiersz , Thomas H. Puzia

We have begun the ExploreNEOs project in which we observe some 700 Near Earth Objects (NEOs) at 3.6 and 4.5 microns with the Spitzer Space Telescope in its Warm Spitzer mode. From these measurements and catalog optical photometry we derive…

We use ALMA measurements of 870 $\mu$m thermal emission from a sample of mid-sized (15-40 km diameter) Jupiter Trojan asteroids to search for high albedo objects in this population. We calculate the diameters and albedos of each object…

地球与行星天体物理 · 物理学 2022-07-06 Anna M. Simpson , Michael E. Brown , Madeline J. Schemel , Bryan J. Butler

We report measured spectral properties for more than 1000 NEOs, representing>5% of the currently discovered population. Thermal flux detected below 2.5 {\mu}m allows us to make albedo estimates for nearly 50 objects, including two comets.…

Near Earth Objects (NEOs) are fragments of remnant primitive bodies that date from the era of Solar System formation. At present, the physical properties and origins of NEOs are poorly understood. We have measured thermal emission from…

We present results for the short-term variability of Binary Trans-Neptunian Objects (BTNOs). We performed CCD photometric observations using the 3.58 m Telescopio Nazionale Galileo, the 1.5 m Sierra Nevada Observatory telescope, and the…

地球与行星天体物理 · 物理学 2014-09-10 A. Thirouin , K. S. Noll , J. L. Ortiz , N. Morales

Context. The trans-neptunian region of the Solar System is populated by a large variety of icy bodies showing great diversity in orbital behavior, size, surface color and composition. One can also note the presence of dynamical families and…

地球与行星天体物理 · 物理学 2015-05-27 Christophe Dumas , Benoit Carry , Daniel Hestroffer , Frederic Merlin

The transneptunian region of the solar system is populated by a wide variety of icy bodies showing great diversity. The dwarf planet (136108) Haumea is among the largest TNOs and displays a highly elongated shape and hosts two moons,…

地球与行星天体物理 · 物理学 2016-09-07 F. Gourgeot , B. Carry , C. Dumas , F. Vachier , F. Merlin , P. Lacerda , M. A. Barucci , J. Berthier

A recent occultation measurement of the dwarf planet Haumea (Ortiz et al. 2017) revealed an elongated shape with the longest axis comparable to Pluto's mean diameter. The chords also indicate a ring around Haumea's equatorial plane, where…

Thermal observations of the Pluto-Charon system acquired by the Herschel Space Observatory in February 2012 are presented. They consist of photometric measurements with the PACS and SPIRE instruments (nine visits to the Pluto system each),…

地球与行星天体物理 · 物理学 2016-03-23 E. Lellouch , P. Santos-Sanz , S. Fornasier , T. Lim , J. Stansberry , E. Vilenius , Cs. Kiss , T. Müller , G. Marton , S. Protopapa , P. Panuzzo , R. Moreno

Precise atmospheric observations have been made for a growing sample of warm Neptunes. Here we investigate the correlations between these observations and a large number of system parameters to show that, at 95% confidence, the amplitude of…

地球与行星天体物理 · 物理学 2017-12-13 Ian J. M. Crossfield , Laura Kreidberg