_version_ 1866908818101764096
author Micheli, Marco
Devogèle, Maxime
Denneau, Larry
Ryan, Eileen V.
Ryan, William H.
Pravec, Petr
Hornoch, Kamil
Kučáková, Hana
Fatka, Petr
Brucker, Melissa J.
Lejoly, Cassandra
Moskovitz, Nicholas
Granvik, Mikael
Gray, Zuri
Fedorets, Grigori
Djupvik, Anlaug Amanda
Fuls, Carson
Rankin, David
Wierzchoś, Kacper
Gray, Bill
Lister, Tim
Wainscoat, Richard J.
Weryk, Robert
Hainaut, Olivier R.
Spoto, Federica
Veres, Peter
Rivkin, Andrew S.
Holler, Bryan J.
Burdanov, Artem Y.
de Wit, Julien
Farnocchia, Davide
Rudawska, Regina
Peleato, Eduardo Alonso
Ocaña, Francisco
Tonry, John
Audenaert, Jeroen
Faggioli, Laura
Gianotto, Francesco
Fenucci, Marco
Conversi, Luca
Moissl, Richard
author_facet Micheli, Marco
Devogèle, Maxime
Denneau, Larry
Ryan, Eileen V.
Ryan, William H.
Pravec, Petr
Hornoch, Kamil
Kučáková, Hana
Fatka, Petr
Brucker, Melissa J.
Lejoly, Cassandra
Moskovitz, Nicholas
Granvik, Mikael
Gray, Zuri
Fedorets, Grigori
Djupvik, Anlaug Amanda
Fuls, Carson
Rankin, David
Wierzchoś, Kacper
Gray, Bill
Lister, Tim
Wainscoat, Richard J.
Weryk, Robert
Hainaut, Olivier R.
Spoto, Federica
Veres, Peter
Rivkin, Andrew S.
Holler, Bryan J.
Burdanov, Artem Y.
de Wit, Julien
Farnocchia, Davide
Rudawska, Regina
Peleato, Eduardo Alonso
Ocaña, Francisco
Tonry, John
Audenaert, Jeroen
Faggioli, Laura
Gianotto, Francesco
Fenucci, Marco
Conversi, Luca
Moissl, Richard
contents The discovery of 2024 YR4 presented the planetary defense community with the most significant impact threat in almost two decades, reaching level 3 on the Torino scale. The community, now mature and well-organized, responded with a global observational effort. Astrometric measurements, forming the basis for orbital refinement and impact prediction, were a central component of this response. In this paper, we present the astrometric data collected by the international community, from the time of discovery until the object became too faint for all existing observational assets, including JWST. We also discuss the coordination role played by the International Asteroid Warning Network, and the importance of publicly available image archives to enable precovery searches.
format Preprint
id arxiv_https___arxiv_org_abs_2602_06890
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert
Micheli, Marco
Devogèle, Maxime
Denneau, Larry
Ryan, Eileen V.
Ryan, William H.
Pravec, Petr
Hornoch, Kamil
Kučáková, Hana
Fatka, Petr
Brucker, Melissa J.
Lejoly, Cassandra
Moskovitz, Nicholas
Granvik, Mikael
Gray, Zuri
Fedorets, Grigori
Djupvik, Anlaug Amanda
Fuls, Carson
Rankin, David
Wierzchoś, Kacper
Gray, Bill
Lister, Tim
Wainscoat, Richard J.
Weryk, Robert
Hainaut, Olivier R.
Spoto, Federica
Veres, Peter
Rivkin, Andrew S.
Holler, Bryan J.
Burdanov, Artem Y.
de Wit, Julien
Farnocchia, Davide
Rudawska, Regina
Peleato, Eduardo Alonso
Ocaña, Francisco
Tonry, John
Audenaert, Jeroen
Faggioli, Laura
Gianotto, Francesco
Fenucci, Marco
Conversi, Luca
Moissl, Richard
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
The discovery of 2024 YR4 presented the planetary defense community with the most significant impact threat in almost two decades, reaching level 3 on the Torino scale. The community, now mature and well-organized, responded with a global observational effort. Astrometric measurements, forming the basis for orbital refinement and impact prediction, were a central component of this response. In this paper, we present the astrometric data collected by the international community, from the time of discovery until the object became too faint for all existing observational assets, including JWST. We also discuss the coordination role played by the International Asteroid Warning Network, and the importance of publicly available image archives to enable precovery searches.
title Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert
topic Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2602.06890