Hubble Astrometry for the Local Group and Beyond in the 2030s
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2026
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| author | Sohn, S. Tony Bennet, Paul McKinnon, Kevin Andrew van der Marel, Roeland P. Libralato, Mattia Vitral, Eduardo Patel, Ekta Watkins, Laura L. del Pino, Andres Bellini, Andrea Griggio, Massimo Fardal, Mark A. Kallivayalil, Nitya Warfield, Jack T. Gilbert, Karoline M. Guhathakurta, Puragra Weisz, Daniel Wetzel, Andrew Pace, Andrew B. Pawlowski, Marcel S. Simon, Joshua D. Besla, Gurtina Tollerud, Erik Ou, Xiaowei Ahvazi, Niusha Bonaca, Anna |
| author_facet | Sohn, S. Tony Bennet, Paul McKinnon, Kevin Andrew van der Marel, Roeland P. Libralato, Mattia Vitral, Eduardo Patel, Ekta Watkins, Laura L. del Pino, Andres Bellini, Andrea Griggio, Massimo Fardal, Mark A. Kallivayalil, Nitya Warfield, Jack T. Gilbert, Karoline M. Guhathakurta, Puragra Weisz, Daniel Wetzel, Andrew Pace, Andrew B. Pawlowski, Marcel S. Simon, Joshua D. Besla, Gurtina Tollerud, Erik Ou, Xiaowei Ahvazi, Niusha Bonaca, Anna |
| contents | Hubble's long, stable astrometric baseline creates a rare opportunity for discovery in the Local Group and beyond. Many nearby galaxies, streams, and star clusters already have archival first-epoch imaging in hand, so future HST observations over the next decade can turn those data into precise proper motions. For many Milky Way satellites, existing measurements already constrain orbital motion at a useful level, but HST still offers a path to full 3D kinematics, internal motions, and more distant systems where current data remain insufficient. That opens the window to dynamical studies inaccessible through line-of-sight velocities alone, revealing orbital histories, internal kinematics, environmental processing, and the dark-matter structure of nearby galaxies. This white paper identifies HST astrometry as an opportunity to capitalize on archival baselines by completing long-baseline measurements where first epochs already exist, establishing new first epochs where critical gaps remain, and assembling a legacy sample for future JWST, Roman, and HWO-era follow-up. The result will be a transformative dataset for the Local Group and Local Volume, driving discovery now while laying the groundwork for the next generation of dynamical studies for resolved stellar populations. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_24191 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Hubble Astrometry for the Local Group and Beyond in the 2030s Sohn, S. Tony Bennet, Paul McKinnon, Kevin Andrew van der Marel, Roeland P. Libralato, Mattia Vitral, Eduardo Patel, Ekta Watkins, Laura L. del Pino, Andres Bellini, Andrea Griggio, Massimo Fardal, Mark A. Kallivayalil, Nitya Warfield, Jack T. Gilbert, Karoline M. Guhathakurta, Puragra Weisz, Daniel Wetzel, Andrew Pace, Andrew B. Pawlowski, Marcel S. Simon, Joshua D. Besla, Gurtina Tollerud, Erik Ou, Xiaowei Ahvazi, Niusha Bonaca, Anna Instrumentation and Methods for Astrophysics Astrophysics of Galaxies Hubble's long, stable astrometric baseline creates a rare opportunity for discovery in the Local Group and beyond. Many nearby galaxies, streams, and star clusters already have archival first-epoch imaging in hand, so future HST observations over the next decade can turn those data into precise proper motions. For many Milky Way satellites, existing measurements already constrain orbital motion at a useful level, but HST still offers a path to full 3D kinematics, internal motions, and more distant systems where current data remain insufficient. That opens the window to dynamical studies inaccessible through line-of-sight velocities alone, revealing orbital histories, internal kinematics, environmental processing, and the dark-matter structure of nearby galaxies. This white paper identifies HST astrometry as an opportunity to capitalize on archival baselines by completing long-baseline measurements where first epochs already exist, establishing new first epochs where critical gaps remain, and assembling a legacy sample for future JWST, Roman, and HWO-era follow-up. The result will be a transformative dataset for the Local Group and Local Volume, driving discovery now while laying the groundwork for the next generation of dynamical studies for resolved stellar populations. |
| title | Hubble Astrometry for the Local Group and Beyond in the 2030s |
| topic | Instrumentation and Methods for Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2605.24191 |