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Record W4414870679 · doi:10.1051/0004-6361/202556498

A high geometric albedo and small size for the Haumea cluster member (24835) 1995 SM <sub>55</sub> determined from a stellar occultation and photometric observations

2025· article· en· W4414870679 on OpenAlexaff
J. L. Ortiz, N. Morales, B. Sicardy, F. L. Rommel, F. Braga-Ribas, Y. Kılıç, E. Fernández-Valenzuela, J. L. Rizos, B. E. Morgado, Luan Machado Catani, M. Kretlow, J. M. Gómez-Limón, J. Desmars, P. Santos-Sanz, O. Erece, İbrahim Aköz, K. Uluç, S. Kaspi, A. Marciniak, Vlad Turcu, Dan Moldovan, A. Şonka, Elisabeta Petrescu, Dan Alin Nedelcu, Çağlayan Nehir, R. Morales, R. Duffard, D. Souami, W. Thuillot, J. I. B. Camargo, R. Vieira-Martins, J. Lecacheux, A. Álvarez-Candal, M. Assafin, G. Benedetti-Rossi, A. Gomes-Junior, R. C. Boufleur, U. Hopp, Claus Goessl, M. Schmidt, A. Takey, A.M. Abdelaziz, H. Mikuž, Andrej Mohar, J. Skvarč, O. Schreurs, M. Lecossois, T. Janik, M. N. Bagiran, Simon Ek, Sinan Aliş, Fuat Korhan YELKENCİ, Mert Acar, Nóra Takács, Róbert Szakáts, András Pál, J. Manek, Bogdan Alexandru Dumitru, K. Gazeas, F. Ursache, D. Nardiello, V. Nascimbeni, M. Rottenborn, Э. Сонбас, W. Ogłoza, Alessandro Nastasi, S. Leonini, M. Conti, P. Rosi, Luz Marina Tinjaca Ramirez, L. Bellizi, Alessandro Marchini, G. Verna, Arif Solmaz, M. Tekeş, D. Antuszewicz, Daniele Pica, D. Ilić, M. Grozdanovic, L. Stoian, P. Bacci, M. Maestripieri, G. Krannich, R. Bacci, Metin Altan, K. Hornoch, R. Nesci, F. Ciabattari, Gy. M. Szabó, J. Kovács, Z. Garai, Zs. Bora, P. Zelený, B. Gaehrken, M. Fiedler, L. Curelaru, S. Ion, R. K. Schaefer, J. Kubánek, P. Delinčák, S. Kalkan

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsNational Capital Commission
Fundersnot available
KeywordsOccultationAlbedo (alchemy)Geometric albedoAngular diameterAbsolute magnitudeSolar SystemCluster (spacecraft)

Abstract

fetched live from OpenAlex

Context . Trans-Neptunian objects (TNOs) are thought to be some of the most ancient and primitive bodies in our Solar System. Understanding their basic physical properties is crucial to unraveling their origin and the evolution of the outer Solar System beyond Neptune. Stellar occultations are a highly effective and sensitive method of studying these distant and faint objects, allowing us to gather essential information about their physical characteristics. (24835) 1995 SM 55 is one of the few members of the Haumea orbital cluster and, therefore, is an especially relevant body to study within the TNO population. Aims . The main objectives of the present work are to determine the projected size, absolute magnitude, and geometric albedo of 1995 SM 55 and to analyze the results compared to Haumea. Methods . We predicted a stellar occultation by this TNO for February, 25, 2024, carried out a specific campaign to observe the occultation, and derived the projected size and shape from the occultation observations using an elliptical fit to the occultation chords. We also analyzed a large set of photometric observations of (24835) 1995 SM 55 to obtain the absolute magnitude and the rotational period. Finally, we combined these results to derive the geometric albedo of this TNO. Results . The occultation was successfully detected from seven instruments located at five different sites; 33 other sites reported negative detections. Using an elliptical fit to the occultation chords, we determined the size and shape of the limb of (24835) 1995 SM 55 during the occultation: an ellipse with semi-axes (104.3 ± 0.4) × (83.5 ± 0.5) km. The area-equivalent diameter ( D eq,A ) for this ellipse is 186.7 ± 1.8 km. This is consistent with the upper limit of 250 km estimated from Herschel Observatory thermal data. From our photometric observations, we derived an absolute magnitude ( H V ) of 4.55 ± 0.03, a phase slope parameter of 0.04 ± 0.02 mag/deg, and a V − R value of 0.37 ± 0.05. The rotational variability has a maximum peak-to-valley amplitude (∆ m ) of 0.05 mag, but we could not derive an unambiguous rotational period. Combining the projected size from the occultation with the absolute photometry, we obtained a geometric albedo in the V band ( p V ) of 0.80 ± 0.04 for 1995 SM 55 . This value is remarkably high for a TNO and somewhat higher than that of Haumea, but consistent with the concept that 1995 SM 55 is a member of the orbital cluster of Haumea.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.029
Threshold uncertainty score0.057

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.013
GPT teacher head0.204
Teacher spread0.191 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations0
Published2025
Admission routes1
Has abstractyes

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