Stellar occultations enable milliarcsecond astrometry for Trans-Neptunian objects and Centaurs
arXiv:2010.12708 · doi:10.1051/0004-6361/202039054
Abstract
Trans-Neptunian objects (TNOs) and Centaurs are remnants of our planetary system formation, and their physical properties have invaluable information for evolutionary theories. Stellar occultation is a ground-based method for studying these small bodies and has presented exciting results. These observations can provide precise profiles of the involved body, allowing an accurate determination of its size and shape. The goal is to show that even single-chord detections of TNOs allow us to measure their milliarcsecond astrometric positions in the reference frame of the Gaia second data release (DR2). Accurated ephemerides can then be generated, allowing predictions of stellar occultations with much higher reliability. We analyzed data from stellar occultations to obtain astrometric positions of the involved bodies. The events published before the Gaia era were updated so that the Gaia DR2 catalog is the reference. Previously determined sizes were used to calculate the position of the object center and its corresponding error with respect to the detected chord and the International Celestial Reference System (ICRS) propagated Gaia DR2 star position. We derive 37 precise astrometric positions for 19 TNOs and 4 Centaurs. Twenty-one of these events are presented here for the first time. Although about 68\% of our results are based on single-chord detection, most have intrinsic precision at the submilliarcsecond level. Lower limits on the diameter and shape constraints for a few bodies are also presented as valuable byproducts. Using the Gaia DR2 catalog, we show that even a single detection of a stellar occultation allows improving the object ephemeris significantly, which in turn enables predicting a future stellar occultation with high accuracy. Observational campaigns can be efficiently organized with this help, and may provide a full physical characterization of the involved object.
arXiv comment16 pages, 28 figures. The manuscript was accepted and is to be published
References in corpus (36)
- Gaia Data Release 2. Summary of the contents and survey properties
- The Gaia mission
- Statistical Study of the Early Solar System's Instability with 4, 5 and 6 Giant Planets
- A ring system detected around the Centaur (10199) Chariklo
- The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation
- "TNOs are Cool": A survey of the trans-Neptunian region X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations
- Gaia Data Release 2: The Celestial reference frame (Gaia-CRF2)
- Simulations of the Population of Centaurs I: The Bulk Statistics
- Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object
- Possible ring material around centaur (2060) Chiron
- "TNOs are Cool": A Survey of the Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
- "TNOs are Cool": A survey of the trans-Neptunian region VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
- The Geology and Geophysics of Kuiper Belt Object (486958) Arrokoth
- TNOs are Cool: A survey of the trans-Neptunian region V. Physical characterization of 18 Plutinos using Herschel PACS observations
- Thermal Properties of Centaurs Asbolus and Chiron
- Orbit determination of Transneptunian objects and Centaurs for the prediction of stellar occultations
- Size and shape of Chariklo from multi-epoch stellar occultations
- "TNOs are Cool": A survey of the trans-Neptunian region -- VII. Size and surface characteristics of (90377) Sedna and 2010 EK139
- Size and Shape Constraints of (486958) Arrokoth from Stellar Occultations
- Study of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features
- The thermal emission of Centaurs and Trans-Neptunian objects at millimeter wavelengths from ALMA observations
- The structure of Chariklo's rings from stellar occultations
- Results from the 2014 November 15th multi-chord stellar occultation by the TNO (229762) 2007 UK
- Trans-Neptunian objects and Centaurs at thermal wavelengths
- "TNOs are Cool": A survey of the trans-Neptunian region XIV. Size/albedo characterization of the Haumea family observed with Herschel and Spitzer
- Candidate stellar occultations by large trans-neptunian objects up to 2015
- Results from a triple chord stellar occultation and far-infrared photometry of the trans-Neptunian object (229762) 2007 UK126
- A multi-chord stellar occultation by the large trans-Neptunian object (174567) Varda
- A stellar occultation by Vanth, a satellite of (90482) Orcus
- Neptune Trojans and Plutinos: colors, sizes, dynamics, and their possible collisions
- The large Trans-Neptunian Object 2002 TC from combined stellar occultation, photometry and astrometry data
- Pluto's ephemeris from ground-based stellar occultations (1988-2016)
- The HST Lightcurve of (486958) 2014 MU69
- The trans-Neptunian object (84922) 2003 VS2 through stellar occultations
- Alignments Of Black Holes With Their Warped Accretion Disks And Episodic Lifetimes Of Active Galactic Nuclei
- A digital video system for observing and recording occultations
Cited by in corpus (17)
- SORA: Stellar Occultation Reduction and Analysis
- Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020
- Constraints on (2060) Chiron's size, shape, and surrounding material from the November 2018 and September 2019 stellar occultations
- Stellar occultations by Trans-Neptunian Objects
- Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation
- Asteroid astrometry by stellar occultations: Accuracy of the existing sample from orbital fitting
- Differential aperture photometry and digital coronagraphy with PRAIA
- A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS
- Investigating the formation of small Solar System objects using stellar occultations by satellites: present, future and its use to update satellite orbits
- Astrometry with PRAIA
- The trans-Neptunian object (119951) 2002 KX14 revealed via multiple stellar occultations
- Reaching sub-millisecond accuracy in stellar occultations and artificial satellites tracking
- Asteroid sizes determined with thermophysical model and stellar occultations
- Discovery of a dwarf planet candidate in an extremely wide orbit: 2017 OF201
- Constraining the size, shape, and albedo of the large Trans-Neptunian Object (28978) Ixion with multi-chord stellar occultations
- Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data
- A high geometric albedo and small size of the Haumea cluster member (24835) 1995 SM55 from a stellar occultation and photometric observations