Light Curves of Trojan Asteroids using TRAPPIST telescopes
Miny, Héloïse
Promotor(s) :
Jehin, Emmanuel
Date of defense : 25-Jun-2025/27-Jun-2025 • Permalink : http://hdl.handle.net/2268.2/22969
Details
| Title : | Light Curves of Trojan Asteroids using TRAPPIST telescopes |
| Author : | Miny, Héloïse
|
| Date of defense : | 25-Jun-2025/27-Jun-2025 |
| Advisor(s) : | Jehin, Emmanuel
|
| Committee's member(s) : | Grodent, Denis
Sluse, Dominique
Ferrais, Marin
|
| Language : | English |
| Number of pages : | 70 |
| Keywords : | [en] Trojans [en] asteroids [en] light curves |
| Discipline(s) : | Physical, chemical, mathematical & earth Sciences > Space science, astronomy & astrophysics |
| Institution(s) : | Université de Liège, Liège, Belgique |
| Degree: | Master en sciences spatiales, à finalité approfondie |
| Faculty: | Master thesis of the Faculté des Sciences |
Abstract
[en] This thesis presents a photometric and astrometric examination of the Jupiter Tro-
jan asteroids (3063) Makhaon, (12929) Periboea, (3708) Socus, (11509) Thersilochos,
and (3793) Leonteus. Light curves were obtained using the TRAPPIST telescopes,
and their amplitudes, rotation periods, and shape properties were analyzed. All of
the objects had rotation periods between around 6 and 12 hours, and their modest
amplitudes suggested spheroidal to moderately elongated forms. Spectral slopes re-
vealed a mostly D-type taxonomy based on BVRI color indices, which is consistent
with red and organic matter-rich surfaces. Orbital elements were calculated using
astrometric data and the Find Orb program to confirm their Trojan nature. These
findings add to our understanding of the variety of Trojan composition, shape, and
spin and offer important background information for upcoming exploration missions
like NASA’s Lucy.
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