_version_ 1866912942309507072
author Rizos, J. L.
Ortiz, J. L.
Rommel, F. L.
Sicardy, B.
Morales, N.
Santos-Sanz, P.
Fernández-Valenzuela, E.
Desmars, J.
Souami, D.
Kretlow, M.
Alvarez-Candal, A.
Gómez-Limón, J. M.
Duffard, R.
Kilic, Y.
Morales, R.
Holler, B. J.
Vara-Lubiano, M.
Marciniak, A.
Kashuba, V.
Koshkin, N.
Kashuba, S.
Pal, A.
Szabó, G. M.
Derekas, A.
Szigeti, L.
Ellington, C.
Schreurs, O.
Mottola, S.
Iglesias-Marzoa, R.
Maícas, N.
Galindo-Guil, F. J.
Organero, F.
Ana, L.
Getrost, K.
Nikitin, V.
Verbiscer, A.
Skrutskie, M.
Gray, Candace
Malacarne, M.
Jacques, C.
Cacella, P.
Canales, O.
Lafuente, D.
Calavia, S.
Oncins, Ch.
Assafin, M.
Braga-Ribas, F.
Camargo, J. I. B.
Gomes-Júnior, A. R.
Morgado, B.
Gradovski, E.
Vieira-Martins, R.
Colas, F.
Tekes, M.
Erece, O.
Kaplan, M.
Schweizer, A.
Kubanek, J.
author_facet Rizos, J. L.
Ortiz, J. L.
Rommel, F. L.
Sicardy, B.
Morales, N.
Santos-Sanz, P.
Fernández-Valenzuela, E.
Desmars, J.
Souami, D.
Kretlow, M.
Alvarez-Candal, A.
Gómez-Limón, J. M.
Duffard, R.
Kilic, Y.
Morales, R.
Holler, B. J.
Vara-Lubiano, M.
Marciniak, A.
Kashuba, V.
Koshkin, N.
Kashuba, S.
Pal, A.
Szabó, G. M.
Derekas, A.
Szigeti, L.
Ellington, C.
Schreurs, O.
Mottola, S.
Iglesias-Marzoa, R.
Maícas, N.
Galindo-Guil, F. J.
Organero, F.
Ana, L.
Getrost, K.
Nikitin, V.
Verbiscer, A.
Skrutskie, M.
Gray, Candace
Malacarne, M.
Jacques, C.
Cacella, P.
Canales, O.
Lafuente, D.
Calavia, S.
Oncins, Ch.
Assafin, M.
Braga-Ribas, F.
Camargo, J. I. B.
Gomes-Júnior, A. R.
Morgado, B.
Gradovski, E.
Vieira-Martins, R.
Colas, F.
Tekes, M.
Erece, O.
Kaplan, M.
Schweizer, A.
Kubanek, J.
contents (119951) 2002 KX14 is a large classical TNO with limited previous observations and unresolved questions regarding its physical properties. Five stellar occultations by 2002 KX14 were observed from 2020 to 2023, involving multiple telescopes across different locations in Europe and the Americas. The five occultations resulted in 15 positive chords, accurately measuring the 2002 KX14's shape and size. The projected ellipse has semi-major and semi-minor axes of $241.0 \pm 7.2$ km and $157.1 \pm 5.2$ km, respectively, corresponding to an average area-equivalent diameter of $389.2 \pm 8.7$ km. The geometric albedo was estimated at $11.9 \pm 0.7\%$.
format Preprint
id arxiv_https___arxiv_org_abs_2503_19179
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The trans-Neptunian object (119951) 2002 KX14 revealed via multiple stellar occultations
Rizos, J. L.
Ortiz, J. L.
Rommel, F. L.
Sicardy, B.
Morales, N.
Santos-Sanz, P.
Fernández-Valenzuela, E.
Desmars, J.
Souami, D.
Kretlow, M.
Alvarez-Candal, A.
Gómez-Limón, J. M.
Duffard, R.
Kilic, Y.
Morales, R.
Holler, B. J.
Vara-Lubiano, M.
Marciniak, A.
Kashuba, V.
Koshkin, N.
Kashuba, S.
Pal, A.
Szabó, G. M.
Derekas, A.
Szigeti, L.
Ellington, C.
Schreurs, O.
Mottola, S.
Iglesias-Marzoa, R.
Maícas, N.
Galindo-Guil, F. J.
Organero, F.
Ana, L.
Getrost, K.
Nikitin, V.
Verbiscer, A.
Skrutskie, M.
Gray, Candace
Malacarne, M.
Jacques, C.
Cacella, P.
Canales, O.
Lafuente, D.
Calavia, S.
Oncins, Ch.
Assafin, M.
Braga-Ribas, F.
Camargo, J. I. B.
Gomes-Júnior, A. R.
Morgado, B.
Gradovski, E.
Vieira-Martins, R.
Colas, F.
Tekes, M.
Erece, O.
Kaplan, M.
Schweizer, A.
Kubanek, J.
Earth and Planetary Astrophysics
(119951) 2002 KX14 is a large classical TNO with limited previous observations and unresolved questions regarding its physical properties. Five stellar occultations by 2002 KX14 were observed from 2020 to 2023, involving multiple telescopes across different locations in Europe and the Americas. The five occultations resulted in 15 positive chords, accurately measuring the 2002 KX14's shape and size. The projected ellipse has semi-major and semi-minor axes of $241.0 \pm 7.2$ km and $157.1 \pm 5.2$ km, respectively, corresponding to an average area-equivalent diameter of $389.2 \pm 8.7$ km. The geometric albedo was estimated at $11.9 \pm 0.7\%$.
title The trans-Neptunian object (119951) 2002 KX14 revealed via multiple stellar occultations
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2503.19179