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Using data from the Infrared Array Camera on the Spitzer Space Telescope, we present photometric observations of a sample of 100 trans-Neptunian objects (TNOs) beyond 2.2 {\mu}m. These observations, collected with two broad-band filters…

The thermal emission of transneptunian objects (TNO) and Centaurs has been observed at mid- and far-infrared wavelengths - with the biggest contributions coming from the Spitzer and Herschel space observatories-, and the brightest ones also…

地球与行星天体物理 · 物理学 2020-01-22 Thomas Müller , Emmanuel Lellouch , Sonia Fornasier

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

\ Nitrous oxide (N$_2$O) ice is likely to exist in trans-Neptunian objects such as Pluto and Triton, potentially formed through ultraviolet (UV) radiation from the Sun or cosmic ray irradiation of N$_2$ and CO ices. However, the…

地球与行星天体物理 · 物理学 2025-04-04 Daiki Takama , Ryoichi Koga , Shohei Negishi , Biao Zhao , Yuan Li , Yasuhiro Hirahara , Fumiyuki Ito

Water is abundant in natural environments but the form it resides in planetary interiors remains uncertain. We report combined synchrotron X-ray diffraction and optical spectroscopy measurements of H2O in the laser-heated diamond anvil cell…

Near-Earth objects (NEOs) are excellent laboratories for testing processes that affect airless bodies, as well as informing us about Solar System history. Though most NEOs are nominally anhydrous because they formed inside the Solar System…

地球与行星天体物理 · 物理学 2026-02-03 Lauren McGraw , Cristina Thomas , Josh Emery , Andy Rivkin

It has been implicitly assumed that ices on grains in molecular clouds and proto planetary disks are formed by homogeneous layers regardless of their composition or crystallinity. To verify this assumption, we observed the H2O deposition…

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

A group of trans-Neptunian objects (TNO) are dynamically related to the dwarf planet 136108 Haumea. Ten of them show strong indications of water ice on their surfaces, are assumed to have resulted from a collision, and are accepted as the…

Orcus is an intermediate-size 1000km-scale Kuiper Belt Object in 3:2 mean-motion resonance with Neptune, in an orbit very similar to that of Pluto. We present visible and near-infrared photometry and spectroscopy obtained with the Keck…

地球与行星天体物理 · 物理学 2015-05-19 Audrey Delsanti , Frédéric Merlin , Aurélie Guilbert , James Bauer , Bin Yang , Karen J. Meech

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…

地球与行星天体物理 · 物理学 2015-05-27 S. D. Benecchi , K. S. Noll , D. C. Stephens , W. M. Grundy , J. Rawlins

We present a new near-infrared photometric system for detection of water ice and methane ice in the solar system. The system consists of two medium-band filters in the K-band region of the near-infrared, which are sensitive to water ice and…

地球与行星天体物理 · 物理学 2015-05-27 Chadwick A. Trujillo , Scott S. Sheppard , Emily L. Schaller

Trans-Neptunian objects (TNOs) contain the most primitive and thermally least-processed materials from the early accretional phase of the solar system. They allow us to study interrelations between various classes of small bodies, their…

天体物理学 · 物理学 2009-11-13 S. Bagnulo , I. Belskaya , K. Muinonen , G. P. Tozzi , M. A. Barucci , L. Kolokolova , S. Fornasier

Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend the role of such ices in the chemistry and evolution of dense molecular clouds and comets, it is necessary to understand the freeze-out,…

天体物理学 · 物理学 2009-11-06 Helen J. Fraser , Mark P. Collings , Martin R. S. McCoustra , David A. Williams

We search for frozen water and its processing around young stellar objects (YSOs of class I/II). We try to detect potential, regional differences in water ice evolution within YSOs, which is relevant to understanding the chemical structure…

地球与行星天体物理 · 物理学 2017-08-30 Alexander A. Schegerer , Sebastian Wolf

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

The crystalline state of water ice in the Solar System depends on the temperature history of the ice and the influence of energetic particles to which it has been exposed. We measured the infrared absorption spectra of amorphous and…

天体物理学 · 物理学 2011-03-31 Weijun Zheng , David Jewitt , Ralf I. Kaiser

We present variability measurements and partial light curves of Trans-Neptunian Objects (TNOs) from a two-night pilot study using Hyper Suprime-Cam (HSC) on the Subaru Telescope (Maunakea, Hawai'i, USA). Subaru's large aperture (8-m) and…

Aims. In this paper we investigate the detectability of the molecular oxygen in icy dust grain mantles towards astronomical objects. Methods. We present a systematic set of experiments with O2-H2O ice mixtures designed to disentangle how…

天体物理仪器与方法 · 物理学 2018-11-28 B. Müller , B. M. Giuliano , L. Bizzocchi , A. I. Vasyunin , P. Caselli

We examine a large collection of low resolution near-infrared spectra of Kuiper belt objects and centaurs in an attempt to understand the presence of water ice in the Kuiper belt. We find that water ice on the surface of these objects…

地球与行星天体物理 · 物理学 2015-06-04 M. E. Brown , E. L. Schaller , W. C. Fraser
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