elib
DLR-Header
DLR-Logo -> http://www.dlr.de
DLR Portal Home | Imprint | Privacy Policy | Contact | Deutsch
Fontsize: [-] Text [+]

Photometry and model of near-Earth asteroid 2021 DW1 from one apparition

Kwiatkowski, T. and Koleńczuk, P. and Kryszczynska, A. and Oszkiewicz, D. A. and Kamiński, K. and Kamińska, M. K. and Troianskyi, V. and Skiff, B. and Moskowitz, N. and Kashuba, V. and Kim, M.-J. and Kim, T. and Mottola, S. and Santana-Ros, T. and Kluwak, T. and Buzzi, L. and Bacci, P. and Birtwhistle, P. and Miles, R. and Chatelain, J. (2021) Photometry and model of near-Earth asteroid 2021 DW1 from one apparition. Astronomy & Astrophysics. EDP Sciences. doi: 10.1051/0004-6361/202142013. ISSN 0004-6361.

[img] PDF - Only accessible within DLR - Postprint version (accepted manuscript)
2MB

Abstract

Aims. Very small asteroids (VSAs, objects with diameters smaller than about 150 m) can be spun up by the YORP effect to rotation periods as short as tens of seconds. This effect has been observed for many of them. It is also hypothesised, that in the same process their spin axes are asymptotically drawn to the position perpendicular to the orbital plane. So far this effect has been observed only for one VSA and needs further verification. For that, spin axes of several other VSAs should be determined by observing their brightness variations at many different positions on the sky. Methods. On 4 March 2021 at 9 UTC a 30-m in diameter near-Earth asteroid 2021 DW1 passed the Earth at a distance of 570 000 km, reaching the maximum brightness of V = 14.6 mag. We observed it photometrically from 2 March, when it was visible at V = 16.5 mag, until 7 March (V = 18.2 mag). During that time 2021 DW1 swept a 170◦long arc in the northern sky, spanning solar phase angles in the range from 36◦to 86◦. This made it an excellent target for physical characterisation, including spin axis and shape derivation. Results. Convex inversion of the asteroid lightcurves gives a sidereal period of rotation Psid = 0.013760 ±0.000001 h, and two solutions for the spin axis ecliptic coordinates: (A) λ1 = 57◦±10◦,β1 = 29◦±10◦and (B) λ2 = 67◦±10◦,β2 = −40◦±10◦. The magnitude-phase curve can be fitted with a standard H, G function with H = 24.8 ±0.5 mag and an assumed G = 0.24. The asteroid colour indices are g −i = 0.79 ±0.01 mag, and i −z = 0.01 ±0.02 mag which indicates an S taxonomic class, with an average geometric albedo pV = 0.23 ±0.02. The asteroid effective diameter, derived from H and pV , is Deff = 30 ±10 m.Conclusions. It was found that the inclination of the spin axis of 2021 DW1 is not perpendicular to the orbital plane (obliquity e = 54◦±10◦or e = 123◦±10◦). More spin axes of VSAs should be determined to check, if 2021 DW1 is an exception or a typical case.

Item URL in elib:https://elib.dlr.de/146866/
Document Type:Article
Additional Information:Bisher nur online erschienen.
Title:Photometry and model of near-Earth asteroid 2021 DW1 from one apparition
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Kwiatkowski, T.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Koleńczuk, P.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Kryszczynska, A.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Oszkiewicz, D. A.Astronomical Observatory Institute, Faculty of Physics, A. Mickiewicz University, Słoneczna 36, 60-286 Poznań, PolandUNSPECIFIEDUNSPECIFIED
Kamiński, K.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Kamińska, M. K.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Troianskyi, V.Astronomical Observatory, Poznan, PolandUNSPECIFIEDUNSPECIFIED
Skiff, B.Lowell Observatory, Flagstaff, AZ 86001, USAUNSPECIFIEDUNSPECIFIED
Moskowitz, N.Lowell Observatory, Flagstaff, AZ 86001, USAUNSPECIFIEDUNSPECIFIED
Kashuba, V.Astronomical Observatory of Odessa I.I.Mechnikov National University, Odessa, UkraineUNSPECIFIEDUNSPECIFIED
Kim, M.-J.Korea Astronomy & Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of KoreaUNSPECIFIEDUNSPECIFIED
Kim, T.National Youth Space Center, Goheung, Jeollanam-do, 59567, KoreaUNSPECIFIEDUNSPECIFIED
Mottola, S.UNSPECIFIEDhttps://orcid.org/0000-0002-0457-3872UNSPECIFIED
Santana-Ros, T.Astronomical Observatory Institute, Faculty of Physics, A. Mickiewicz University, Słoneczna 36, 60-286 Poznań, PolandUNSPECIFIEDUNSPECIFIED
Kluwak, T.Platanus Observatory, Lusówko, PolandUNSPECIFIEDUNSPECIFIED
Buzzi, L.Schiaparelli Astronomical Observatory, Varese, ItalyUNSPECIFIEDUNSPECIFIED
Bacci, P.Osservatorio di San Marcello Pistoiese, GAMP Gruppo Astrofili Montagna Pistoiese, ItalyUNSPECIFIEDUNSPECIFIED
Birtwhistle, P.Great Shefford Observatory, Berkshire, United KingdomUNSPECIFIEDUNSPECIFIED
Miles, R.British Astronomical Association, Burlington House, Piccadilly, London, United KingdomUNSPECIFIEDUNSPECIFIED
Chatelain, J.Las Cumbres Observatory, Goleta, CA 93117, USAUNSPECIFIEDUNSPECIFIED
Date:4 October 2021
Journal or Publication Title:Astronomy & Astrophysics
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
DOI:10.1051/0004-6361/202142013
Publisher:EDP Sciences
ISSN:0004-6361
Status:Published
Keywords:asteroids – photometric observations – period, spin axis, shape modelling
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - LUCY
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Geodesy
Deposited By: Mottola, Dr.phys. Stefano
Deposited On:07 Dec 2021 09:26
Last Modified:20 Oct 2023 08:30

Repository Staff Only: item control page

Browse
Search
Help & Contact
Information
electronic library is running on EPrints 3.3.12
Website and database design: Copyright © German Aerospace Center (DLR). All rights reserved.