_version_ 1866911943616364544
author Buie, Marc W.
Spencer, John R.
Porter, Simon B.
Benecchi, Susan D.
Parker, Alex H.
Stern, S. Alan
Belton, Michael
Binzel, Richard P.
Borncamp, David
DeMeo, Francesca
Fabbro, S.
Fuentes, Cesar
Furusawa, Hisanori
Fuse, Tetsuharu
Gay, Pamela L.
Gwyn, Stephen
Holman, Matthew J.
Karoji, H.
Kavelaars, J. J.
Kinoshita, Daisuke
Miyazaki, Satoshi
Mountain, Matt
Noll, Keith S.
Osip, David J.
Petit, Jean-Marc
Reid, Neill I.
Sheppard, Scott S.
Showalter, Mark
Steffl, Andrew J.
Sterner, Ray E.
Tajitsu, Akito
Tholen, David J.
Trilling, David E.
Weaver, Harold A.
Verbiscer, Anne J.
Wasserman, Lawrence H.
Yamashita, Takuji
Yanagisawa, Toshifumi
Yoshida, Fumi
Zangari, Amanda M.
author_facet Buie, Marc W.
Spencer, John R.
Porter, Simon B.
Benecchi, Susan D.
Parker, Alex H.
Stern, S. Alan
Belton, Michael
Binzel, Richard P.
Borncamp, David
DeMeo, Francesca
Fabbro, S.
Fuentes, Cesar
Furusawa, Hisanori
Fuse, Tetsuharu
Gay, Pamela L.
Gwyn, Stephen
Holman, Matthew J.
Karoji, H.
Kavelaars, J. J.
Kinoshita, Daisuke
Miyazaki, Satoshi
Mountain, Matt
Noll, Keith S.
Osip, David J.
Petit, Jean-Marc
Reid, Neill I.
Sheppard, Scott S.
Showalter, Mark
Steffl, Andrew J.
Sterner, Ray E.
Tajitsu, Akito
Tholen, David J.
Trilling, David E.
Weaver, Harold A.
Verbiscer, Anne J.
Wasserman, Lawrence H.
Yamashita, Takuji
Yanagisawa, Toshifumi
Yoshida, Fumi
Zangari, Amanda M.
contents Following the Pluto fly-by of the New Horizons spacecraft, the mission provided a unique opportunity to explore the Kuiper Belt in-situ. The possibility existed to fly-by a Kuiper Belt object (KBO) as well as to observe additional objects at distances closer than are feasible from earth-orbit facilities. However, at the time of launch no KBOs were known about that were accessible by the spacecraft. In this paper we present the results of 10 years of observations and three uniquely dedicated efforts -- two ground-based using the Subaru Suprime Camera, the Magellan MegaCam and IMACS Cameras, and one with the Hubble Space Telescope -- to find such KBOs for study. In this paper we overview the search criteria and strategies employed in our work and detail the analysis efforts to locate and track faint objects in the galactic plane. We also present a summary of all of the KBOs that were discovered as part of our efforts and how spacecraft targetability was assessed, including a detailed description of our astrometric analysis which included development of an extensive secondary calibration network. Overall, these efforts resulted in the discovery of 89 KBOs including 11 which became objects for distant observation by New Horizons and (486958) Arrokoth which became the first post-Pluto fly-by destination.
format Preprint
id arxiv_https___arxiv_org_abs_2403_04927
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The New Horizons Extended Mission Target: Arrokoth Search and Discovery
Buie, Marc W.
Spencer, John R.
Porter, Simon B.
Benecchi, Susan D.
Parker, Alex H.
Stern, S. Alan
Belton, Michael
Binzel, Richard P.
Borncamp, David
DeMeo, Francesca
Fabbro, S.
Fuentes, Cesar
Furusawa, Hisanori
Fuse, Tetsuharu
Gay, Pamela L.
Gwyn, Stephen
Holman, Matthew J.
Karoji, H.
Kavelaars, J. J.
Kinoshita, Daisuke
Miyazaki, Satoshi
Mountain, Matt
Noll, Keith S.
Osip, David J.
Petit, Jean-Marc
Reid, Neill I.
Sheppard, Scott S.
Showalter, Mark
Steffl, Andrew J.
Sterner, Ray E.
Tajitsu, Akito
Tholen, David J.
Trilling, David E.
Weaver, Harold A.
Verbiscer, Anne J.
Wasserman, Lawrence H.
Yamashita, Takuji
Yanagisawa, Toshifumi
Yoshida, Fumi
Zangari, Amanda M.
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Following the Pluto fly-by of the New Horizons spacecraft, the mission provided a unique opportunity to explore the Kuiper Belt in-situ. The possibility existed to fly-by a Kuiper Belt object (KBO) as well as to observe additional objects at distances closer than are feasible from earth-orbit facilities. However, at the time of launch no KBOs were known about that were accessible by the spacecraft. In this paper we present the results of 10 years of observations and three uniquely dedicated efforts -- two ground-based using the Subaru Suprime Camera, the Magellan MegaCam and IMACS Cameras, and one with the Hubble Space Telescope -- to find such KBOs for study. In this paper we overview the search criteria and strategies employed in our work and detail the analysis efforts to locate and track faint objects in the galactic plane. We also present a summary of all of the KBOs that were discovered as part of our efforts and how spacecraft targetability was assessed, including a detailed description of our astrometric analysis which included development of an extensive secondary calibration network. Overall, these efforts resulted in the discovery of 89 KBOs including 11 which became objects for distant observation by New Horizons and (486958) Arrokoth which became the first post-Pluto fly-by destination.
title The New Horizons Extended Mission Target: Arrokoth Search and Discovery
topic Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2403.04927