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Related papers: Compositional study of trans-Neptunian objects at …

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We investigate whether the surfaces of the classical moons of Uranus are compositionally stratified, with a thin veneer of mostly tiny H2O ice grains (<= 2 micron diameters) mantling a lower layer composed of larger grains of H2O ice, dark…

JWST NIRSpec IFU (2.9-5.3 mu) and MIRI MRS (4.9-28.5 mu) observations were performed on both the leading and trailing hemispheres of Ganymede with a spectral resolution of ~2700. Reflectance spectra show signatures of water ice, CO2 and…

Superconducting thin films of niobium have been extensively employed in transmon qubit architectures. Although these architectures have demonstrated remarkable improvements in recent years, further improvements in performance through…

We study the dust present in 56 Galactic planetary nebulae (PNe) through their iron depletion factors, their C/O abundance ratios (in 51 objects), and the dust features that appear in their infrared spectra (for 33 objects). Our sample…

Solar and Stellar Astrophysics · Physics 2015-06-18 Gloria Delgado-Inglada , Mónica Rodríguez

In this work, we present 0.7-5.0 {\mu}m spectra of eight Neptunian Trojans (NTs) as observed by the JWST's NIRSpec instrument. The reddest NT, 2013 VX30, exhibits a unique spectrum with strong absorption features between 3 - 4 {\mu}m, while…

Earth and Planetary Astrophysics · Physics 2025-06-11 Larissa Markwardt , Hsing Wen Lin , Bryan J. Holler , David W. Gerdes , Fred C. Adams , Renu Malhotra , Kevin J. Napier

We use 1.4-4.6 micron multi-band photometry of the small inner Uranian and Neptunian satellites obtained with the James Webb Space Telescope's near-infrared imager NIRCam to characterize their surface compositions. We find that the…

Earth and Planetary Astrophysics · Physics 2025-06-02 Matthew Belyakov , M. Ryleigh Davis , Zachariah Milby , Ian Wong , Michael E. Brown

The most pristine remnants of the Solar system's planet formation epoch orbit the Sun beyond Neptune, the small bodies of the trans-Neptunian object populations. The bulk of the mass is in ~100 km objects, but objects at smaller sizes have…

Earth and Planetary Astrophysics · Physics 2024-02-19 Andrew Shannon , Alain Doressoundiram , Françoise Roques , Bruno Sicardy , Quentin Kral

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.…

A technique based on neutron activation has been developed for an extremely high sensitivity analysis of trace elements in organic materials. Organic materials are sealed in plastic or high purity quartz and irradiated at the HFIR and MITR.…

High Energy Physics - Experiment · Physics 2009-11-07 Z. Djurcic , D. Glasgow , L-W. Hu , R. D. McKeown , A. Piepke , R. Swinney , B. Tipton

The generic properties of compact objects made of two different fluids of dark matter are studied in a scale invariant approach. We investigate compact objects with a core-shell structure, where the two fluids are separated, and with mixed…

General Relativity and Quantum Cosmology · Physics 2023-03-01 Marie Cassing , Alexander Brisebois , Muhammad Azeem , Jürgen Schaffner-Bielich

We explore the chemistry and observability of nitrogen dominated atmospheres for ultra-short-period super-Earths. We base the assumption, that super-Earths could have nitrogen filled atmospheres, on observations of 55 Cnc e that favour a…

Earth and Planetary Astrophysics · Physics 2020-03-25 Mantas Zilinskas , Yamila Miguel , Paul Mollière , Shang-Min Tsai

Space missions to NEOs are being planned at all major space agencies, and recently a manned mission to an NEO was announced as a NASA goal. Efforts to find and select suitable targets (plus backup targets) are severely hampered by our lack…

We present the results of an archival search for Trans-neptunian objects (TNOs) in an ecliptic field observed with Subaru in 2002. The depth of the search allowed us to find 20 new TNOs with magnitudes between R=24 and 27. We fit a double…

Astrophysics · Physics 2011-02-11 Cesar I. Fuentes , Matthew R. George , Matthew J. Holman

\ 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…

Earth and Planetary Astrophysics · Physics 2025-04-04 Daiki Takama , Ryoichi Koga , Shohei Negishi , Biao Zhao , Yuan Li , Yasuhiro Hirahara , Fumiyuki Ito

Planets smaller than Neptune and larger than Earth make up the majority of the discovered exoplanets. Those with H$_2$-rich atmospheres are prime targets for atmospheric characterization. The transition between the two main classes,…

Earth and Planetary Astrophysics · Physics 2021-12-08 Shang-Min Tsai , Hamish Innes , Tim Lichtenberg , Jake Taylor , Matej Malik , Katy Chubb , Raymond Pierrehumbert

We report on our first results from a mid-infrared spectroscopic study of ISM features in a sample of deeply obscured ULIRG nuclei using the InfraRed Spectrograph (IRS) on the Spitzer Space Telescope. The spectra are extremely rich and…

The sensitivity of ALMA makes it possible to detect thermal mm/submm emission from small/distant Solar System bodies at the sub-mJy level. Measured fluxes are primarily sensitive to the objects' diameters, but deriving precise sizes is…

Earth and Planetary Astrophysics · Physics 2017-12-06 E. Lellouch , R. Moreno , T. Müller , S. Fornasier , P. Santos-Sanz , A. Moullet , M. Gurwell , J. Stansberry , R. Leiva , B. Sicardy , B. Butler , J. Boissier

Most known trans-Neptunian objects (TNOs) gravitationally scattering off the giant planets have orbital inclinations consistent with an origin from the classical Kuiper belt, but a small fraction of these "scattering TNOs" have inclinations…

We discover two infrared objects that show deep absorption features of H2O, CO2, and CO ices in the AKARI/Infrared Camera (IRC) slit-less spectroscopic survey of the Galactic plane in 2.5--13 micron. Both objects are located neither in…

Astrophysics of Galaxies · Physics 2021-08-11 Takashi Onaka , Tomoyuki Kimura , Itsuki Sakon , Takashi Shimonishi

We present in this paper mid-infrared (5-8~$\mu$m) spectroscopy toward the massive young binary W3~IRS~5, using the EXES spectrometer in high-resolution mode ($R\sim$50,000) from the NASA Stratospheric Observatory for Infrared Astronomy…