Asteroid Taxonomy from Cluster Analysis of Spectrometry and Albedo
arXiv:2203.11229 · doi:10.1051/0004-6361/202243587
Abstract
The classification of the minor bodies of the Solar System based on observables has been continuously developed and iterated over the past 40 years. While prior iterations followed either the availability of large observational campaigns or new instrumental capabilities opening new observational dimensions, we see the opportunity to improve primarily upon the established methodology. We developed an iteration of the asteroid taxonomy which allows the classification of partial and complete observations (i.e. visible, near-infrared, and visible-near-infrared spectrometry) and which reintroduces the visual albedo into the classification observables. The resulting class assignments are given probabilistically, enabling the uncertainty of a classification to be quantified. We built the taxonomy based on 2983 observations of 2125 individual asteroids, representing an almost tenfold increase of sample size compared with the previous taxonomy. The asteroid classes are identified in a lower-dimensional representation of the observations using a mixture of common factor analysers model. We identify 17 classes split into the three complexes C, M, and S, including the new Z-class for extremely-red objects in the main belt. The visual albedo information resolves the spectral degeneracy of the X-complex and establishes the P-class as part of the C-complex. We present a classification tool which computes probabilistic class assignments within this taxonomic scheme from asteroid observations. The taxonomic classifications of 6038 observations of 4526 individual asteroids are published. The ability to classify partial observations and the reintroduction of the visual albedo provide a taxonomy which is well suited for the current and future datasets of asteroid observations, in particular provided by the Gaia, MITHNEOS, NEO Surveyor, and SPHEREx surveys.
Published in Astronomy and Astrophysics. The table of asteroid classifications and the templates of the defined taxonomic classes are available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/665/A26
References in corpus (41)
- Initial Performance of the NEOWISE Reactivation Mission
- Solar System evolution from compositional mapping of the asteroid belt
- Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS
- Thermal inertia of main belt asteroids smaller than 100 km from IRAS data
- Main Belt Asteroids with WISE/NEOWISE: Near-Infrared Albedos
- Visible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families
- Multiple and Fast: The Accretion of Ordinary Chondrite Parent Bodies
- Thermophysical modeling of asteroids from WISE thermal infrared data - Significance of the shape model and the pole orientation uncertainties
- NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
- Olivine-dominated A-type asteroids in the Main Belt: Distribution, Abundance and Relation to Families
- Different origins or different evolutions? Decoding the spectral diversity among C-type asteroids
- The Composition of M-type asteroids II: Synthesis of spectroscopic and radar observations
- Asteroid phase curves from ATLAS dual-band photometry
- Thermal Infrared Observations of Asteroid (99942) Apophis with Herschel
- Physical and dynamical properties of the main belt triple asteroid (87) Sylvia
- Survey Simulations of a New Near-Earth Asteroid Detection System
- The Albedo Distribution of Near Earth Asteroids
- The debiased compositional distribution of MITHNEOS: Global match between the near-Earth and main-belt asteroid populations and excess of D-type Near-Earth Objects
- NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos
- Physical characterisation of near-Earth asteroid (1620) Geographos. Reconciling radar and thermal-infrared observations
- Adaptive optics and lightcurve data of asteroids: twenty shape models and information content analysis
- Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene
- Near-Earth asteroids spectroscopic survey at Isaac Newton Telescope
- Discovery of two TNO-like bodies in the asteroid belt
- More chips off of Asteroid (4) Vesta: characterization of eight Vestoids and their HED meteorite analogs
- Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data
- The visible and near-infrared spectra of asteroids in cometary orbits
- Spectral properties of the largest asteroids associated with Taurid Complex
- NEOSurvey 1: Initial results from the Warm Spitzer Exploration Science Survey of Near Earth Object Properties
- A common origin for dynamically associated near-Earth asteroid pairs
- Spectral reflectance analysis of type 3 carbonaceous chondrites and search for their asteroidal parent bodies
- The olivine-dominated composition of the Eureka family of Mars Trojan asteroids
- Similar origin for low- and high-albedo Jovian Trojans and Hilda asteroids ?
- A data-driven model of nucleosynthesis with chemical tagging in a lower-dimensional latent space
- Investigating S-type asteroid surfaces through reflectance spectra of Ordinary Chondrites
- Thermophysical Modeling of 20 Themis Family Asteroids with WISE/NEOWISE Observations
- m spectra of Hilda asteroids
- Spectral characterisation of 14 V-type candidate asteroids from the MOVIS catalogue
- Nature of bright C-complex asteroids
- A thermophysical and dynamical study of the Hildas (1162) Larissa and (1911) Schubart
- Space Weathering within C-Complex Main Belt Asteroid Families
Cited by in corpus (32)
- Euclid. I. Overview of the Euclid mission
- Asteroid Kamo`oalewa's journey from the lunar Giordano Bruno crater to Earth 1:1 resonance
- SsODNet: The Solar system Open Database Network
- Combined spin orientation and phase function of asteroids
- Debris Disk Color with the Hubble Space Telescope
- Spectral analysis of basaltic asteroids observed by the Gaia space mission
- Gaia search for early-formed andesitic asteroidal crusts
- Euclid: Identification of asteroid streaks in simulated images using deep learning
- Rotation periods of asteroids from light curves of TESS data
- Observations of two super fast rotator NEAs: 2021 NY and 2022 AB
- Deficit of primitive compositions in binary asteroids and pairs
- Spectral analogues of Barbarian asteroids among CO and CV chondrites
- The Distribution of Highly Red-sloped Asteroids in the Middle and Outer Main Belt
- Simultaneous visible spectrophotometry of interstellar object 3I/ATLAS with Seimei/TriCCS
- Compositional properties of planet-crossing asteroids from astronomical surveys
- (433) Eros and (25143) Itokawa surface properties from reflectance spectra
- Optical spectropolarimetry of large C-complex asteroids: polarimetric evidence for heterogeneous surface compositions
- Near-Ultraviolet Absorption Distribution of Primitive Asteroids from Spectrophotometric Surveys
- Gaia and IRTF abundance of A-type main belt asteroids
- Gaia DR3 asteroid reflectance spectra: L-type families, memberships, and ages
- Characterization of of (98943) 2001 CC, the target of Hayabusa2
- HyperScout-H: the hyperspectral imager for the ESA Hera mission
- Multi-epoch spectro-photometric characterization of the minimoon 2024 PT in the visible and near-infrared
- Primitive asteroids in the main belt, Cybele, and Hilda populations from Gaia DR3
- The possible dual nature of the asteroid (12499) 1998 FR47
- Orbits of very distant asteroid satellites
- The dependence of the asteroid rotation on their composition
- On the rotation of M-type asteroids: statistical evidence for higher rotation rates
- Composition and Space Weathering Characteristics of Tianwen-2 Mission's First Target Near-Earth Asteroid (469219) Kamo`oalewa
- Surface Properties, Orbital Dynamics, and Thermophysical Modeling of the Primitive Asteroid (269) Justitia
- Speckle observations of the binary asteroid (22) Kalliope with C2PU/PISCO
- An ancient L- type family associated to (460) Scania in the Middle Main Belt as revealed by Gaia DR3 spectra