Physical models of ten asteroids from an observers' collaboration network
Josef Durech
(1)
,
Mikko Kaasalainen
(2)
,
A. Marciniak
(3)
,
W. H. Allen
(4)
,
Raoul Behrend
(5)
,
C. Bembrick
(6)
,
T. Bennett
(7)
,
L. Bernasconi
(8)
,
Jerôme Berthier
(9, 10)
,
G. Bolt
,
S. Boroumand
(11)
,
L. Crespo da Silva
(11)
,
R. Crippa
(12)
,
M. Crow
(13)
,
R. Durkee
(14)
,
R. Dymock
,
M. Fagas
(3)
,
M. Fauerbach
(7)
,
S. Fauvaud
(15, 16)
,
M. Frey
(17)
,
R. Goncalves
(18)
,
R. Hirsch
(3)
,
D. Jardine
(19)
,
K. Kaminski
(3)
,
R. Koff
(20)
,
T. Kwiatkowski
(3)
,
Arturo Lopez-Ariste
(21)
,
F. Manzini
(12)
,
T. Michalowski
(3)
,
R. Pacheco
(21)
,
Ming Pan
(11)
,
F. Pilcher
(19)
,
R. Poncy
,
D. P. Pray
(22)
,
W. Pych
(23)
,
R. Roy
(24)
,
G. Santacana
(15)
,
S. Slivan
(17)
,
Stefano Sposetti
(25)
,
R. Stephens
(26)
,
B. Warner
(27)
,
M. Wolf
(1)
1
UK -
Univerzita Karlova [Praha, Česká republika] = Charles University [Prague, Czech Republic]
2 Department of Mathematics and Statistics, Rolf Nevanlinna Institute, University of Helsinki
3 Astronomical Observatory, Adam Mickiewicz University
4 Vintage Lane Observatory
5 Observatoire Astronomique de l'Université de Genève
6 Mount Tarana Observatory
7 Florida Gulf Coast University
8 Observatoire des Engarouines
9 IMCCE - Institut de Mécanique Céleste et de Calcul des Ephémérides
10 GAP - Groupe Astrométrie et Planétologie
11 EAPS - Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge]
12 Stazzione Astronomica di Sozzago
13 The WW Crow Observatory,
14 Shed of Science Observatory
15 Association AstroQueyras
16 GEOS - Groupe européen d’observation stellaire
17 Department of Astronomy, Whitin Observatory, Wellesley College
18 Observatório Astronómico de Linhaceira
19 Illinois College
20 Antelope Hills Observatory, 980 Antelope Drive West, Bennett
21 Observatori Astronomic de Consell
22 Carbuncle Hill Observatory
23 CAMK - Centrum Astronomiczne im. M. Kopernika, Warszawa
24 Observatoire de Blauvac
25 Observatorio di Gnosca
26 Goat Mountain Astronomical Research Station
27 Palmer Divide Observatory, Colorado Springs
2 Department of Mathematics and Statistics, Rolf Nevanlinna Institute, University of Helsinki
3 Astronomical Observatory, Adam Mickiewicz University
4 Vintage Lane Observatory
5 Observatoire Astronomique de l'Université de Genève
6 Mount Tarana Observatory
7 Florida Gulf Coast University
8 Observatoire des Engarouines
9 IMCCE - Institut de Mécanique Céleste et de Calcul des Ephémérides
10 GAP - Groupe Astrométrie et Planétologie
11 EAPS - Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge]
12 Stazzione Astronomica di Sozzago
13 The WW Crow Observatory,
14 Shed of Science Observatory
15 Association AstroQueyras
16 GEOS - Groupe européen d’observation stellaire
17 Department of Astronomy, Whitin Observatory, Wellesley College
18 Observatório Astronómico de Linhaceira
19 Illinois College
20 Antelope Hills Observatory, 980 Antelope Drive West, Bennett
21 Observatori Astronomic de Consell
22 Carbuncle Hill Observatory
23 CAMK - Centrum Astronomiczne im. M. Kopernika, Warszawa
24 Observatoire de Blauvac
25 Observatorio di Gnosca
26 Goat Mountain Astronomical Research Station
27 Palmer Divide Observatory, Colorado Springs
Résumé
Aims:We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys.
Methods: The lightcurve inversion method was used to derive spin states and shape models of the asteroids.
Results: We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred.
Methods: The lightcurve inversion method was used to derive spin states and shape models of the asteroids.
Results: We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred.
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