The PHEMU21 catalogue and astrometric results of the observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made in 2021

Author:

Emelyanov N12,Arlot J-E2,Anbazhagan P3,André P4,Bardecker J5,Canaud G6,Coliac J F7,De Elias Cantalapiedra J8,Ellington C K9,Fernandez J M10,Forbes M11,Gazeas K12,Gault D13,George T14,Gourdon F15,Herald D16,Huber D17,Iglesias-Marzoa R18,Izquierdo J8,Jorba Lloveras R8,Kerr S16,Lasala A19,Le Guen P20,Leroy A6,Lutz M21,Maley P22,Mannchen T21,Mari J M17,Maury A1718,Newman J16,Palafouta S12ORCID,Prieto Gallego J8,Roger P15,Röschli D23,Selvakumar G3,Serra V21,Stuart P24,Turchenko M125,Vasundhara R26,Velasco E827

Affiliation:

1. Sternberg Astronomical Institute, Lomonosov Moscow State University , Russia

2. Institut de mécanique céleste et de calcul des éphémérides-Observatoire de Paris , PSL, UMR 8028 CNRS, UPMC, USTL, 77 avenue Denfert-Rochereau, F-75014 Paris, France

3. Vainu Bappu Observatory, Indian Institute of Astrophysics , 635701 Kavalur, Tamil Nadu, India

4. IOTA-ES, Société Astronomique de France , Adagio Belesta Observatory, Club d’astronomie de Quint-Fonsegrives, F-31570 Sainte Foy d’Aigrefeuille, France

5. IOTA , Gardnerville, Nevada, USA

6. Uranoscope de l’Ile de France , F-77220 Gretz-Armainvilliers, France

7. OABAC : Observatoire pour l’Astronomie des Binaires et l’Astronomie Collaborative , Marseille, France

8. Agrupación Astronómica de Madrid , E-28029 Madrid, Spain

9. Maastricht Science Programme , NL-6229 Maastricht, Netherlands

10. Astronomía Sevilla , Seville, Spain

11. Occultation section RASNZ, Manor Park Observatory, , Lower Hutt 5019, New Zealand

12. Section of Astrophysics, Astronomy and Mechanics, Department of Physics, National and Kapodistrian University of Athens , GR-15784 Zografos, Athens, Greece

13. 22 Booker Road , Hawkesbury Heights, N.S.W. 2777, Australia

14. IOTA , Scottsdale, AZ USA

15. OAGC Observatoire Astronomique du Gros Cerveau , Rte du Gros Cerveau F-83190 Ollioules, France

16. Trans-Tasman Occultation Alliance , Murrumbateman Observatory, Australia

17. GAPRA , F-06160 Antibes-Juan-les-Pins, France

18. Centro de Estudios de Física del Cosmos de Aragón, Javalambre Astrophysical Observatory , E-44001, Teruel, Spain

19. AAHU , Astronomical group of Huesca, Zaragoza, Spain

20. Observatoire du Pic des Fées , 26 bis All. des Pinsons, F-83400 Hyères, Toulon, France

21. Baden-Wuerttemberg Cooperative State University (DHBW) Ravensburg Campus Friedrichshafen; Fallenbrunnen 2 , D-88045 Friedrichshafen, Germany

22. IOTA and NASA Johnson Space Center Astronomical Society , Carefree, AZ, USA

23. Cademario Observatory , Switzerland

24. International Occultation Timing Association (IOTA) , Fountain Hills, AZ 85269, USA

25. Caucasian Mountain Observatory of the SAI of Moscow State University, Karachay-Cherkess Republic , Kichi-Balyk village, 369388 Russia

26. Indian Institute of Astrophysics , Bangalore 560034, Karnataka, India

27. Department of Theoretical Condensed Matter Physics, Facultad de Ciencias, Universidad Autonoma de Madrid, , E-28049 Madrid, Spain

Abstract

ABSTRACT 2021 was the year of Jupiter’s equinox, that is the Sun and the Earth passed through the equatorial plane of the planet and therefore the orbital planes of its main satellites. This occurrence made it possible to observe mutual occultations and eclipses between the satellites. Our former experience shows that observations of such events provide accurate astrometric data that can be used to obtain new information on the dynamics of the Galilean satellites. The observations are a series of photometric measurements of a satellite which are carried out through the organization of a world wide campaign of observations thus maximizing the number and the quality of the data obtained. This work focuses on processing the photometric observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made during the international campaign in 2021. The final goal is to derive new accurate astrometric data. We used an accurate photometric model of mutual events in conjunction with the accuracy of observation. We obtained and processed the 84 light curves obtained during the campaign. As compared with the current best ephemerides, the rms of ‘O–C’ residuals are equal to 49 and 48 mas in right ascension and declination, respectively.

Funder

FP7

CNES

CNRS

ICTS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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