New Horizons

NASA spacecraft launched in 2006

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March 6 2024
2014 OS393
Minor Planet Center published additional observations by New Horizons KBO Search-Subaru, allowing computation of a more reliable orbit through MPEC 2024-E99.
December 2023 New Horizons had discovered approximately 100 Kuiper Belt Objects and closely examined about 20 of them, capturing details about their shape, rotational period, potential moons, and surface composition.
September 2023 NASA announced that beginning in fiscal year 2025, New Horizons will focus on specific heliophysics data, while remaining available for a potential Kuiper belt flyby until 2028.
2021
2014 OS393
Hal Weaver confirmed that the object is a binary system, with two components of similar size located close to each other.
2021 Mission extension period ends, concluding the planned extended observations of Kuiper Belt objects.
April 17 2021 New Horizons reached a distance of 50 astronomical units (AU) from the Sun while remaining fully operational.
2020
2014 OS393
Initial observations of the object's binary nature remained inconclusive.
May 2020 New Horizons observed the dwarf planet Haumea from a distance of 63 AU, continuing its extended mission of studying Kuiper Belt objects.
April 2020 New Horizons was used with Earth telescopes to take pictures of nearby stars Proxima Centauri and Wolf 359, producing the first demonstrable stellar parallax from over 6.4 billion km apart.
November 12 2019
486958 Arrokoth
Official naming ceremony for Arrokoth held at NASA Headquarters, with permission from Pamunkey Indian Tribe elders, and the naming citation published in a Minor Planet Circular.
November 8 2019
486958 Arrokoth
The International Astronomical Union's Minor Planet Center accepted the name 'Arrokoth'.
January 2019
2014 OS393
New Horizons spacecraft passed the Kuiper belt object at a distance of less than 0.1 AU (15 million km, 9.3 million miles), making it the second closest KBO observed by the mission after Arrokoth.
January 9 2019 New Horizons returned to a spin-stabilized mode to prepare for sending the remaining data back to Earth, with a full data download expected to take approximately 20 months.
January 2 2019 Continued transmission of high-priority data from the Arrokoth encounter to Earth.
January 1 2019 New Horizons completed its flyby of Kuiper belt object 486958 Arrokoth (previously nicknamed Ultima Thule).
January 1 2019
486958 Arrokoth
NASA's New Horizons space probe conducted a flyby of Arrokoth, making it the farthest and most primitive object in the Solar System visited by a spacecraft at that time.
December 24 2018 Completion of the official approach phase to Arrokoth.
September 2018
2011 JY31
New Horizons spacecraft conducted distant observations that revealed 2011 JY31 is a binary trans-Neptunian object, with two components in a tight, mutual orbit.
August 2018 NASA used results from New Horizons' Alice instrument to confirm the existence of a 'hydrogen wall' at the outer edges of the Solar System.
August 16 2018 Official approach phase to Arrokoth began. New Horizons made its first detection of Arrokoth from a distance, observing it at magnitude 20 against a stellar background in the constellation Sagittarius.
August 13 2018 Spacecraft transitioned from spin-stabilized mode to three-axis-stabilized mode in preparation for the Arrokoth encounter.
June 5 2018 New Horizons spacecraft was awakened from hibernation at approximately 00:33 UTC to prepare for the Arrokoth encounter approach phase.
April 11 2018
Dorothy
The International Astronomical Union (IAU) officially approved the name 'Dorothy' for the impact crater, naming it after Dorothy Gale from The Wonderful Wizard of Oz.
March 13 2018
486958 Arrokoth
NASA selected 'Ultima Thule' as the nickname for the object following a public suggestion process.
December 5 2017 New Horizons took a calibration image of the Wishing Well cluster from 40.9 AU away, breaking the record for the most distant image ever taken by a spacecraft. The spacecraft then imaged two Kuiper belt objects from close distances of 0.50 and 0.34 AU.
March 12 2017
486958 Arrokoth
Arrokoth was given the permanent minor planet number 486958.
October 25 2016 Last recorded data from the Pluto flyby was received from New Horizons at 21:48 UTC.
July 2016 LORRI camera captured distant images of Quaoar to study its light-scattering properties.
July 1 2016 The New Horizons mission received funding extension through 2021 for further exploration of Kuiper Belt Objects (KBOs), enabling the Kuiper Belt Extended Mission (KEM).
April 7 2016 New Horizons re-imaged KBO 15810 Arawn with the LORRI instrument, refining its location and determining its rotational period of 5.47 hours.
March 30 2016 New Horizons reached the halfway point of transmitting the Pluto flyby data, approximately nine months after the initial flyby.
2015
2014 OS393
New Horizons probe completed its flyby of Arrokoth and began observations of surrounding Kuiper belt objects.
November 4 2015 Completed the final engine firing to adjust the spacecraft's trajectory for the upcoming Kuiper Belt Object flyby.
November 2 2015 New Horizons imaged Kuiper Belt Object (KBO) 15810 Arawn using the LORRI instrument, beginning detailed observations of the object.
October 22 2015 New Horizons spacecraft began a series of course adjustment engine firings to prepare for the Arrokoth flyby.
August 28 2015
2014 OS393
New Horizons team announced the selection of a Kuiper belt object as the next flyby target, eliminating other potential targets.
August 28 2015 NASA selected 486958 Arrokoth (initially known as Ultima Thule) as the flyby target for the New Horizons mission in the Kuiper Belt.
July 2015
Dorothy
The New Horizons space probe discovered the Dorothy crater during its flyby of the Pluto-Charon system, capturing detailed images of the largest known impact basin on Charon.
July 14 2015 New Horizons flew above the surface of Pluto, becoming the first spacecraft to explore the dwarf planet at a distance of 34 AU from the Sun.
July 7 2015 New Horizons resumed scheduled science operations after resolving the software anomaly.
July 5 2015 NASA announced the software problem was a timing flaw involving simultaneous data compression and command sequence copying that overloaded the spacecraft's primary computer.
July 4 2015 New Horizons experienced a software anomaly and entered safe mode due to a timing flaw in a command sequence preparing for the Pluto flyby.
May 11 2015 A hazard search was conducted to look for potential dangers to the spacecraft such as unknown rings or moons, with no additional hazards found.
April 25 2015 Smaller moons Kerberos and Styx were first observed in photos.
April 15 2015 Pluto was imaged showing a possible polar cap.
March 2015
486958 Arrokoth
The Minor Planet Center assigned the provisional designation to Arrokoth.
February 12 2015 NASA released new images of Pluto and its largest moon Charon, taken from January 25 to 31 during the New Horizons probe's approach.
January 15 2015 Spacecraft began its approach phase to Pluto.
January 4 2015 Distant-encounter operations at Pluto began. NASA initiated Pluto imaging using the LORRI imager and Ralph telescope to help mission navigators design course-correcting engine maneuvers.
December 6 2014 New Horizons was brought back online from hibernation mode in preparation for the Pluto encounter, and instrument check-out began.

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This contents of the box above is based on material from the Wikipedia articles 2014 OS393, 486958 Arrokoth, Dorothy (Charonian crater), New Horizons & 2011 JY31, which are released under the Creative Commons Attribution-ShareAlike 4.0 International License.

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