Why the Northern Hemisphere Needs a 30-40m Telescope and the Science at Stake: from Interstellar Visitors to Planetary Defence
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arXiv
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| Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Formato: | Preprint |
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2025
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| 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 |