Color, Composition, and Thermal Environment of Kuiper Belt Object (486958) Arrokoth
arXiv:2002.06720 · doi:10.1126/science.aay3705
Abstract
The outer Solar System object (486958) Arrokoth (provisional designation 2014 MU) has been largely undisturbed since its formation. We study its surface composition using data collected by the New Horizons spacecraft. Methanol ice is present along with organic material, which may have formed through radiation of simple molecules. Water ice was not detected. This composition indicates hydrogenation of carbon monoxide-rich ice and/ or energetic processing of methane condensed on water ice grains in the cold, outer edge of the early Solar System. There are only small regional variations in color and spectra across the surface, suggesting Arrokoth formed from a homogeneous or well-mixed reservoir of solids. Microwave thermal emission from the winter night side is consistent with a mean brightness temperature of 295 K.
arXiv comment31 pages, 8 figures
References in corpus (35)
- Rapid planetesimal formation in turbulent circumstellar discs
- Streaming Instabilities in Protoplanetary Disks
- The effects of snowlines on C/O in planetary atmospheres
- Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune
- The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys
- An Old Disk That Can Still Form a Planetary System
- The Canada-France Ecliptic Plane Survey - Full Data Release: The orbital structure of the Kuiper belt
- "TNOs are Cool": A survey of the trans-Neptunian region X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations
- First detection of gas-phase methanol in a protoplanetary disk
- An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz
- Mass measurements in protoplanetary disks from hydrogen deuteride
- Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object
- Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
- On the Size-Dependence of the Inclination Distribution of the Main Kuiper Belt
- Microscopic simulation of methanol and formaldehyde ice formation in cold dense cores
- Long-Range Reconnaissance Imager on New Horizons
- Evidence for Two Populations of Classical Transneptunian Objects: The Strong Inclination Dependence of Classical Binaries
- Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift
- High Albedos of Low Inclination Classical Kuiper Belt Objects
- CO destruction in protoplanetary disk midplanes: inside versus outside the CO snow surface
- The Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar System: The Compositional Classes of the Kuiper Belt
- The solar nebula origin of (486958) Arrokoth, a primordial contact binary in the Kuiper belt
- Systematic Variations of CO Gas Abundance with Radius in Gas-rich Protoplanetary Disks
- The Properties of Jovian Trojan Asteroids Listed in SDSS Moving Object Catalog 3
- The Geology and Geophysics of Kuiper Belt Object (486958) Arrokoth
- The Correlated Colors of Transneptunian Binaries
- Cometary ices in forming protoplanetary disc midplanes
- The Bimodal Colors of Centaurs and Small Kuiper Belt Objects
- Col-OSSOS: z Band Photometry Reveals Three Distinct TNO Surface Types
- High-Precision Orbit Fitting and Uncertainty Analysis of (486958) 2014 MU69
- A three-phase approach to grain surface chemistry in protoplanetary disks: Gas, ice surfaces and ice mantles of dust grains
- The Small Numbers of Large Kuiper Belt Objects
- Inflight Radiometric Calibration of New Horizons' Multispectral Visible Imaging Camera (MVIC)
- Forming the Cold Classical Kuiper Belt in a light Disk
- Methanol formation in TW Hya and future prospects for detecting larger complex molecules in disks with ALMA
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- CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing
- The solar nebula origin of (486958) Arrokoth, a primordial contact binary in the Kuiper belt
- The Geology and Geophysics of Kuiper Belt Object (486958) Arrokoth
- A Tale of Planet Formation: From Dust to Planets
- On the Origin and Thermal Stability of Arrokoths and Plutos Ices
- The Sublimative Evolution of (486958) Arrokoth
- Discovery of two TNO-like bodies in the asteroid belt
- System-level fractionation of carbon from disk and planetesimal processing
- Sublimation of ices during the early evolution of Kuiper belt objects
- Surface Dynamics, Equilibrium Points and Individual Lobes of the Kuiper Belt Object (486958) Arrokoth
- Photometry of Kuiper Belt Object (486958) Arrokoth from New Horizons LORRI
- Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs
- Dynamical Implantation of Blue Binaries in the Cold Classical Kuiper Belt
- Sublimation as an effective mechanism for flattened lobes of (486958) Arrokoth
- Global Modeling of Nebulae With Particle Growth, Drift, and Evaporation Fronts. III. Redistribution of Refractories and Volatiles
- Simulation of CHOH ice UV photolysis under laboratory conditions
- The fate of particles in the dynamical environment around Kuiper Belt object (486958) Arrokoth
- Infrared action spectroscopy as tool for probing gas-phase dynamics: Protonated Dimethyl Ether, (CH)OH, formed by the reaction of CHOH with CHOH
- Considering contact forces during the formation of planetesimals by gravitational collapse: mutual orbits, spin states, and shapes
- Direct contact binary planetesimal formation from gravitational collapse