Dataciencia

Colección SciELO Chile

VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno

Indexado

WoS	WOS:000361803900149
Scopus	SCOPUS_ID:84941207014

DOI

10.1051/0004-6361/201526626

Año

2015

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and spin of the large asteroid (3) Juno with the all-data asteroid modelling (ADAM) procedure. These data set limits on the plausible range of shape models, yielding reconstructions suggesting that, despite its large size, Juno has sizable unrounded features moulded by non-gravitational processes such as impacts.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

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Dimensions: https://www.dimensions.ai/why-dimensions/

Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Viikinkoski, M.	Hombre	Tampere Univ Technol - Finlandia Tampere University of Technology - Finlandia Tampere University - Finlandia
2	Kaasalainen, Mikko	Hombre	Tampere Univ Technol - Finlandia Tampere University of Technology - Finlandia Tampere University - Finlandia
3	Durech, J.	Hombre	Charles Univ Prague - República Checa Charles University - República Checa
4	Carry, Benoit	Hombre	Univ Lille 1 - Francia UNS - Francia Université des Sciences et Technologies de Lille - Francia Laboratoire Joseph-Louis Lagrange - Francia Institut de Mecanique Celeste et de Calcul des Ephemerides - Francia
5	Marsset, Michael	Hombre	ESO - Chile Aix Marseille Univ - Francia European Southern Observatory Santiago - Chile Laboratoire d'Astrophysique de Marseille - Francia Observatorio Europeo Austral - Chile
6	Fusco, T.	Hombre	Aix Marseille Univ - Francia Off Natl Etud & Rech Aerosp - Francia Laboratoire d'Astrophysique de Marseille - Francia ONERA - Optics Department - Francia ONERA Office National d'Etudes et Recherches Aerospatiales - Francia
7	Dumas, C.	Hombre	ESO - Chile European Southern Observatory Santiago - Chile Observatorio Europeo Austral - Chile
8	Merline, William J.	Hombre	SW Res Inst - Estados Unidos Space Science and Engineering Division - Estados Unidos
9	Yang, Bin	-	ESO - Chile European Southern Observatory Santiago - Chile Observatorio Europeo Austral - Chile
10	Berthier, J.	Hombre	Univ Lille 1 - Francia Université des Sciences et Technologies de Lille - Francia Institut de Mecanique Celeste et de Calcul des Ephemerides - Francia
11	Kervella, P.	Hombre	CNRS - Chile Universidad de Chile - Chile Univ Paris Diderot - Francia LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique - Francia
12	Vernazza, P.	Hombre	Aix Marseille Univ - Francia Laboratoire d'Astrophysique de Marseille - Francia

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 33.33 %
Citas No-identificadas: 66.67 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 33.33 %
Citas No-identificadas: 66.67 %

Financiamiento

Fuente
Grantová Agentura Ceské Republiky
National Aeronautics and Space Administration
W. M. Keck Foundation
Czech Science Foundation
NASA Exoplanet Science Institute
Academy of Finland
GrantovÃ¡ Agentura ÄeskÃ© Republiky

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Agradecimientos

Agradecimiento
Based on observations collected at the European Southern Observatory, Paranal, Chile (prog. ID: 60.A-9379, 086.C-0785), and at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00013.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This research made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This work was supported by the Centre of Excellence in Inverse Problems Research (Academy of Finland). The work of J.D. was supported by the research grant GACR 15-04816S of the Czech Science Foundation.

Agradecimiento

Based on observations collected at the European Southern Observatory, Paranal, Chile (prog. ID: 60.A-9379, 086.C-0785), and at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.

This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00013.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This research made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This work was supported by the Centre of Excellence in Inverse Problems Research (Academy of Finland). The work of J.D. was supported by the research grant GACR 15-04816S of the Czech Science Foundation.