Discovery [1] | |
---|---|
Discovered by | COIAS |
Discovery site | Maunakea |
Discovery date | 23 January 2017 |
Designations | |
(697402) Ao | |
Named after | Ao Manaka [1] (comic/animation character) |
2017 BX232 | |
main-belt | |
Orbital characteristics [1] | |
Epoch 31 March 2024 (JD 2460400.5) | |
Uncertainty parameter 0 | |
Observation arc | 6654 days |
Aphelion | 3.518 AU |
Perihelion | 2.940 AU |
3.229 AU | |
Eccentricity | 0.0895423 |
5.8 yr | |
327.27995° | |
0° 10m 11.416s / day | |
Inclination | 8.94156° |
190.52888° | |
78.85772° | |
Physical characteristics | |
17.09 | |
(697402) Ao, provisional designation 2017 BX232, is an outer main-belt asteroid. It was discovered on 23 January 2017, by the citizen science project Come On! Impacting ASteroids (COIAS) [1] using archival data from the Subaru Telescope, [2] which was first reported to the Minor Planet Center in February 2024. [3]
Ao is an Outer Main-belt Asteroid [4] in a heliocentric orbit with a semi-major axis of about 3.2 AU in a relatively circular orbit with an eccentricity of 0.09 and an inclination of about 9 degrees. It orbits the Sun every 5.8 years. [1]
The first observation of Ao was on 25 March 2006 by Mt. Lemmon Survey. [1] The asteroid was also observed and reported in later years, however, only in late 2016 and 2017, it has been observed for multiple nights in a single opposition, which is how the Minor Planet Center determines the discovery opposition. [5] However, these observations made using Subaru Telescope were not reported until February 2024 through the web-based citizen science project Come On! Impacting ASteroids (COIAS). Between years 2017 and 2024, other observations were also made, none of which provided multiple night observations in a single opposition. Multiple astrometric measurement reports through the COIAS project belonging to observations dated 2017 therefore became the earliest reports of multiple-night observations of the asteroid within a single opposition, determining the discovery observations. The asteroid was located in these images by using a digital blinking and moving object detection method. [6]
After the astrometric measurements belonging to 2017 observations were identified to belong to the same object, a provisional designation 2017 BX232 was assigned to the object. After its orbital uncertainty parameter dropped to 0, the asteroid was numbered (697402) and the discovery credit was assigned to Subaru Telescope and later to the citizen science project COIAS.
For the naming of the asteroid, the COIAS development team and the citizen scientists who have taken part in the astrometric measurements of (697402) has made a discussion. [7] It was decided to name the asteroid after the fictional character Ao Manaka, who appears as a main character in the comic/animation Asteroid in Love created by author Quro. This decision is explained in the naming citation as follows:
Ao Manaka is a character in the comic/animation Asteroid in Love created by Japanese manga artist Quro. Ao and her friends enjoy Earth Science Club activities in their high school with a dream of naming an asteroid “Ao.” The work encouraged many readers to study Earth and planetary sciences with its accurate depiction of celestial objects and geology. [1]
624 Hektor is the largest Jupiter trojan and the namesake of the Hektor family, with a highly elongated shape equivalent in volume to a sphere of approximately 225 to 250 kilometers diameter. It was discovered on 10 February 1907, by astronomer August Kopff at Heidelberg Observatory in southwest Germany, and named after the Trojan prince Hector, from Greek mythology. It has one small 12-kilometer sized satellite, Skamandrios, discovered in 2006.
Comet Elst–Pizarro is a body that displays characteristics of both asteroids and comets, and is the prototype of active asteroids. Its orbit keeps it within the asteroid belt, yet it displayed a dust tail like a comet while near perihelion in 1996, 2001, and 2007.
118401 LINEAR (provisional designation 1999 RE70, comet designation 176P/LINEAR) is an active asteroid and main-belt comet that was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) 1-metre telescopes in Socorro, New Mexico on September 7, 1999. (118401) LINEAR was discovered to be cometary on November 26, 2005, by Henry H. Hsieh and David C. Jewitt as part of the Hawaii Trails project using the Gemini North 8-m telescope on Mauna Kea and was confirmed by the University of Hawaii's 2.2-m (88-in) telescope on December 24–27, 2005, and Gemini on December 29, 2005. Observations using the Spitzer Space Telescope have resulted in an estimate of 4.0±0.4 km for the diameter of (118401) LINEAR.
15810 Arawn (provisional designation 1994 JR1) is a trans-Neptunian object (TNO) from the inner regions of the Kuiper belt, approximately 133 kilometres (83 mi) in diameter. It belongs to the plutinos, the most populous class of resonant TNOs. It was named after Arawn, the ruler of the underworld in Welsh mythology, and was discovered on 12 May 1994, by astronomers Michael Irwin and Anna Żytkow with the 2.5-metre Isaac Newton Telescope at Roque de los Muchachos Observatory in the Canary Islands, Spain.
474640 Alicanto (provisional designation 2004 VN112) is a detached extreme trans-Neptunian object. It was discovered on 6 November 2004, by American astronomer Andrew C. Becker at Cerro Tololo Inter-American Observatory in Chile. It never gets closer than 47 AU from the Sun (near the outer edge of the main Kuiper belt) and averages more than 300 AU from the Sun. Its large eccentricity strongly suggests that it was gravitationally scattered onto its current orbit. Because it is, like all detached objects, outside the current gravitational influence of Neptune, how it came to have this orbit cannot yet be explained. It was named after Alicanto, a nocturnal bird in Chilean mythology.
2577 Litva, provisional designation 1975 EE3, is a Hungarian-type Mars-crosser and rare trinary asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter.
(612584) 2003 QX113 is a large trans-Neptunian object from the scattered disc located in the outermost region of the Solar System. It is one of the most distant objects from the Sun at 60.5 AU. It was discovered by astronomers with the Canada–France Ecliptic Plane Survey at Mauna Kea Observatories, Hawaii, when it was near aphelion on 31 August 2003. It was provisionally designated 2003 QX113.
471143 Dziewanna (provisional designation 2010 EK139) is a trans-Neptunian object in the scattered disc, orbiting the Sun in the outermost region of the Solar System.
(444030) 2004 NT33 is a classical trans-Neptunian object and possible dwarf planet of the Kuiper belt in the outermost region of the Solar System, approximately 450 kilometers in diameter. It was discovered on 13 July 2004, by astronomers at Palomar Observatory, California, United States.
2010 KZ39 is a trans-Neptunian object orbiting the Sun as a detached object in the outer reaches of the Solar System. The object was first observed on 21 May 2010 by astronomers Andrzej Udalski, Scott Sheppard, M. Szymanski and Chad Trujillo at the Las Campañas Observatory in Chile.
(523639) 2010 RE64 (provisional designation 2010 RE64) is a trans-Neptunian object in the scattered disc located in the outermost region of the Solar System, approximately 570 kilometers (350 miles) in diameter. It was discovered on 11 July 2010 by the Pan-STARRS-1 survey at the Haleakala Observatory, Hawaii, in the United States.
2014 RC is a sub-kilometer near-Earth object and Apollo asteroid. The exceptionally fast rotator passed within 0.000267 AU (39,900 km; 24,800 mi) (0.1 lunar distances) of Earth on 7 September 2014. The asteroid is approximately the diameter of the Chelyabinsk meteor, and passed almost as close to Earth as 367943 Duende (2012 DA14) did in 2013.
420356 Praamzius (provisional designation 2012 BX85) is a trans-Neptunian object from the classical Kuiper belt, located in the outermost region of the Solar System, approximately 190–320 kilometers (120–200 miles) in diameter. It was discovered on 23 January 2012, by astronomers Kazimieras Černis and Richard Boyle with the Vatican's VATT at Mount Graham Observatory in Arizona, United States. The cold classical Kuiper belt object is a weak dwarf planet candidate and possibly very red in color. It was named after the chief god Praamžius from Lithuanian mythology.
(674118) 2015 KH162 is a large trans-Neptunian object orbiting in the scattered disc region of the outermost Solar System. First observed in 2015, this minor planet is one of the most distant objects from the Sun at 60.6 AU, or twice as far as Neptune.
(505448) 2013 SA100, provisional designation 2013 SA100 and also known as o3l79, is a trans-Neptunian object from the classical Kuiper belt in the outermost region of the Solar System. It was discovered on 5 August 2013, by astronomer with the Outer Solar System Origins Survey at the Mauna Kea Observatories, Hawaii, in the United States. The classical Kuiper belt object belongs to the hot population and is a weak dwarf planet candidate, approximately 260 kilometers (160 miles) in diameter.
2018 VG18 is a distant trans-Neptunian object (TNO) that was discovered when it was 123 AU (18 billion km; 11 billion mi) from the Sun, more than three times the average distance between the Sun and Pluto. It was discovered on 10 November 2018 by Scott Sheppard, David Tholen, and Chad Trujillo during their search for TNOs whose orbits might be gravitationally influenced by the hypothetical Planet Nine. They announced the discovery of 2018 VG18 on 17 December 2018 and nicknamed the object "Farout" to emphasize its distance from the Sun.
2018 AG37 is a distant trans-Neptunian object and centaur that was discovered 132.2 ± 1.5 AU (19.78 ± 0.22 billion km) from the Sun, farther than any other currently observable known object in the Solar System. Imaged in January 2018 during a search for the hypothetical Planet Nine, the confirmation of this object was announced in a press release in February 2021 by astronomers Scott Sheppard, David Tholen, and Chad Trujillo. The object was nicknamed "FarFarOut" to emphasize its distance from the Sun.
(523764) 2014 WC510 (provisional designation 2014 WC510) is a binary trans-Neptunian object and plutino discovered on 8 September 2011 by the Pan-STARRS survey at the Haleakalā Observatory in Hawaii. It orbits in the Kuiper belt, a region of icy objects orbiting beyond Neptune in the outer Solar System. Astronomers discovered the binary nature of 2014 WC510 when its two components occulted a star on 1 December 2018. The components of the 2014 WC510 binary system, which have diameters of 180 km (110 mi) and 140 km (87 mi), orbit each other at a separation distance of roughly 2,600 km (1,600 mi).
2021 RR205 is an extreme trans-Neptunian object discovered by astronomers Scott Sheppard, David Tholen, and Chad Trujillo with the Subaru Telescope at Mauna Kea Observatory on 5 September 2021. It resides beyond the outer extent of the Kuiper belt on a distant and highly eccentric orbit detached from Neptune's gravitational influence, with a large perihelion distance of 55.5 astronomical units (AU). Its large orbital semi-major axis (~1,000 AU) suggests it is potentially from the inner Oort cloud. 2021 RR205 and 2013 SY99 both lie in the 50–75 AU perihelion gap that separates the detached objects from the more distant sednoids; dynamical studies indicate that such objects in the inner edge this gap weakly experience "diffusion", or inward orbital migration due to minuscule perturbations by Neptune. While Sheppard considers 2021 RR205 a sednoid, researchers Yukun Huang and Brett Gladman do not.
(718492) Quro, provisional designation 2017 FZ233, is a main-belt asteroid. It was discovered on 22 March 2017, by the citizen science project Come On! Impacting ASteroids (COIAS) using archival data from the Subaru Telescope, which was first reported to the Minor Planet Center in 2024.