_version_ 1866917150674911232
author de León, J.
Pinilla-Alonso, N.
Tanga, P.
Souami, D.
Gray, Z.
Alvarez-Candal, A.
Carry, B.
Marcos, R. de la Fuente
Delsanti, A.
La Forgia, F.
Migliorini, A.
Müller, T.
Penttilä, A.
Popescu, M.
Snodgrass, C.
Oszkiewicz, D.
Opitom, C.
Campo-Bagatin, A.
Licandro, J.
Hueso, R.
Lazzarin, M.
Fornasier, S.
Brunetto, R.
Brasón, J. A. de Abol
Juez, J. de Cos
DeMartini, J.
Donaldson, A.
Dorsey, R.
Duffard, R.
Díaz, J. Fernández
de Leániz, F. García
Díaz, R. Hevia
Gómez-Limón, J. M.
Groussin, O.
Álvarez, S. Iglesias
Kohout, T.
Kretlow, M.
Pivert-Jolivet, T. Le
Montero-Vega, M.
Morales, N.
Muinonen, K.
Ortiz, J. L.
Prodan, G. P.
Rizos, J. L.
Robinson, J. E.
Cabo, S. Rodríguez
Rodríguez, J. Rodríguez
Rozek, A.
Santos-Sanz, P.
Tatsumi, E.
Tinaut-Ruano, F.
Villaver, E.
author_facet de León, J.
Pinilla-Alonso, N.
Tanga, P.
Souami, D.
Gray, Z.
Alvarez-Candal, A.
Carry, B.
Marcos, R. de la Fuente
Delsanti, A.
La Forgia, F.
Migliorini, A.
Müller, T.
Penttilä, A.
Popescu, M.
Snodgrass, C.
Oszkiewicz, D.
Opitom, C.
Campo-Bagatin, A.
Licandro, J.
Hueso, R.
Lazzarin, M.
Fornasier, S.
Brunetto, R.
Brasón, J. A. de Abol
Juez, J. de Cos
DeMartini, J.
Donaldson, A.
Dorsey, R.
Duffard, R.
Díaz, J. Fernández
de Leániz, F. García
Díaz, R. Hevia
Gómez-Limón, J. M.
Groussin, O.
Álvarez, S. Iglesias
Kohout, T.
Kretlow, M.
Pivert-Jolivet, T. Le
Montero-Vega, M.
Morales, N.
Muinonen, K.
Ortiz, J. L.
Prodan, G. P.
Rizos, J. L.
Robinson, J. E.
Cabo, S. Rodríguez
Rodríguez, J. Rodríguez
Rozek, A.
Santos-Sanz, P.
Tatsumi, E.
Tinaut-Ruano, F.
Villaver, E.
contents Small Solar system Objects (SSOs) preserve the physical, chemical, and dynamical signatures of the Sun's protoplanetary disk. Upcoming surveys will discover vast numbers of new objects, yet their scientific value will depend on follow-up observations requiring far greater sensitivity and resolution than those currently available. A 30-m class telescope like the Extremely Large Telescope (ELT) will be transformative, but its Southern location will leave significant regions of the sky poorly covered or even non accessible. A Northern 30-40m telescope is therefore essential to achieve full-sky coverage and fully exploit the small body discoveries of the 2030-2050 era, in particular for targets of opportunity or unexpected discoveries, like those of interstellar objects and potentially hazardous asteroids, as well as for distant trans-Neptunian objects and space mission targets.
format Preprint
id arxiv_https___arxiv_org_abs_2512_14785
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Why the Northern Hemisphere Needs a 30-40m Telescope and the Science at Stake: from Interstellar Visitors to Planetary Defence
de León, J.
Pinilla-Alonso, N.
Tanga, P.
Souami, D.
Gray, Z.
Alvarez-Candal, A.
Carry, B.
Marcos, R. de la Fuente
Delsanti, A.
La Forgia, F.
Migliorini, A.
Müller, T.
Penttilä, A.
Popescu, M.
Snodgrass, C.
Oszkiewicz, D.
Opitom, C.
Campo-Bagatin, A.
Licandro, J.
Hueso, R.
Lazzarin, M.
Fornasier, S.
Brunetto, R.
Brasón, J. A. de Abol
Juez, J. de Cos
DeMartini, J.
Donaldson, A.
Dorsey, R.
Duffard, R.
Díaz, J. Fernández
de Leániz, F. García
Díaz, R. Hevia
Gómez-Limón, J. M.
Groussin, O.
Álvarez, S. Iglesias
Kohout, T.
Kretlow, M.
Pivert-Jolivet, T. Le
Montero-Vega, M.
Morales, N.
Muinonen, K.
Ortiz, J. L.
Prodan, G. P.
Rizos, J. L.
Robinson, J. E.
Cabo, S. Rodríguez
Rodríguez, J. Rodríguez
Rozek, A.
Santos-Sanz, P.
Tatsumi, E.
Tinaut-Ruano, F.
Villaver, E.
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Small Solar system Objects (SSOs) preserve the physical, chemical, and dynamical signatures of the Sun's protoplanetary disk. Upcoming surveys will discover vast numbers of new objects, yet their scientific value will depend on follow-up observations requiring far greater sensitivity and resolution than those currently available. A 30-m class telescope like the Extremely Large Telescope (ELT) will be transformative, but its Southern location will leave significant regions of the sky poorly covered or even non accessible. A Northern 30-40m telescope is therefore essential to achieve full-sky coverage and fully exploit the small body discoveries of the 2030-2050 era, in particular for targets of opportunity or unexpected discoveries, like those of interstellar objects and potentially hazardous asteroids, as well as for distant trans-Neptunian objects and space mission targets.
title Why the Northern Hemisphere Needs a 30-40m Telescope and the Science at Stake: from Interstellar Visitors to Planetary Defence
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2512.14785