Lowell Observatory Near-Earth-Object Search

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Lowell Observatory Near-Earth-Object Search
Neo-chart.png
Alternative namesLONEOS OOjs UI icon edit-ltr-progressive.svg
Organization
Observatory code 699   OOjs UI icon edit-ltr-progressive.svg
Location Flagstaff, Coconino County, Arizona
Coordinates 35°12′10″N111°39′52″W / 35.2028°N 111.6644°W / 35.2028; -111.6644
Website asteroid.lowell.edu/asteroid/loneos/loneos.html OOjs UI icon edit-ltr-progressive.svg
Usa edcp relief location map.png
Red pog.svg
Location of Lowell Observatory Near-Earth-Object Search
Minor planets discovered: 22,077 [1]
see List of minor planets § Main index

Lowell Observatory Near-Earth-Object Search (LONEOS) was a project designed to discover asteroids and comets that orbit near the Earth. The project, funded by NASA, was directed by astronomer Ted Bowell of Lowell Observatory in Flagstaff, Arizona. The LONEOS project began in 1993 and ran until the end of February 2008.

Contents

Hardware

LONEOS, in its final configuration, used a 0.6-meter f/1.8 Schmidt telescope, acquired from Ohio Wesleyan University in 1990, and a Lowell-built 16 megapixel CCD detector. This combination of instruments provided a field of view of 2.88 by 2.88 degrees (8.3 square degrees). It had a maximum nightly scan area of about 1,000 square degrees (covered four times). The instrument could cover the entire accessible dark sky in about a month. The CCD has detected asteroids as faint as visual magnitude 19.8 but its typical limiting visual magnitude was 19.3. The instrument is located at Lowell Observatory's dark sky site, Anderson Mesa Station, near Flagstaff, Arizona, US.

Four computers were used. Two were used for frame reductions, one for telescope pointing control and one for camera control. The camera control software had scripting capability and could control all the other computers.

Technique

Asteroids were found by obtaining four pictures (frames) of the same region of sky, each frame temporally separated by 15 to 30 minutes. The set of four frames were then submitted to reduction software which located all star-like sources on the frame and identified sources that moved with asteroid-like motion. The observer visually examined all asteroid detections that had motion different from a typical main-belt asteroid. Human examination was required because most putative NEO detections were not real but some kind of imaging artifact.

All asteroid positions were converted to equatorial coordinates. Various USNO star catalogs [2] were used for this conversion until 2007. Then the Sloan Digital Sky Survey catalog was used, along with supplemental information from the Carlsberg Catalog [3] and the 2MASS catalog. Asteroid brightness was converted to standard visual magnitude. These data, along with the time of the observations, were sent to the Minor Planet Center (MPC) from which they were distributed to the scientific community. Potential near-Earth objects were handled expeditiously so that other observers could locate the asteroid on the same night and make further observations.

Telescope operation was automated to the extent that the survey could be run all night without observer intervention. However, the telescope was seldom operated in the automatic mode because an observer was required to reduce data promptly and to correct any malfunctions that might have occurred.

Discoveries

Number of NEOs detected by various surveys:
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LINEAR

NEAT

Spacewatch

LONEOS
CSS

Pan-STARRS

NEOWISE

All others NEA by survey.png
Number of NEOs detected by various surveys:
   LINEAR
   NEAT
   Spacewatch
  LONEOS
   CSS
   Pan-STARRS
   NEOWISE
   All others

As of 2017, LONEOS is credited by the Minor Planet Center with the discovery of 22,077 minor planets between 1998 and 2008. The discoveries include main-belt asteroids, near-Earth Objects (NEO) and Mars-crossers. [1] During the period of LONEOS operation, several other NASA funded NEO searches were underway (number of discoveries in parentheses): [1]

Amateur observers made a significant contribution during this time with independent NEO discoveries and by performing follow-up observations of recent discoveries made by the NASA sponsored surveys. [4]

NEO-discovery statistics

The table below lists the number of discoveries made by LONEOS each year of operation. Asteroids thought to be larger than one kilometer in diameter were used as benchmarks in assessing survey completeness. Hence, some table elements have two numbers separated by a slash. The second number represents the number of discoveries larger than one kilometer. The column labeled "Asteroid Observations" is the number of observations sent to the Minor Planet Center. Each asteroid was typically observed four times (once per frame) each night. [5]

YearAsteroid Observations NEAs PHAs Atens Apollos Amors Comets
1998122,5507/400/03/24/21
1999128,22014/752/26/36/26
2000271,23738/1043/018/517/56
2001626,97642/1194/017/421/77
2002407,06421/433/19/09/33
2003720,52854/10175/126/323/62
2004716,15239/495/022/412/04
2005820,60942/486/015/121/38
2006679,92719/120/011/18/02
2007630,46912/022/04/06/03
200888,9531/000/01/00/00
Total5,212,685289/555930/4131/23127/2842

A complete list of LONEOS NEO observations can be found at the NeoDys [6] web site.

Other science

The LONEOS frame archive provides a data set with wide spatial and temporal sky coverage. Other investigators have used these characteristics to produce the following research papers and presentations.

Highlights

LONEOS staff

Lowell staff:

Collaborators:

See also

Related Research Articles

<span class="mw-page-title-main">Lincoln Near-Earth Asteroid Research</span> American astronomical survey for identifying and tracking near-Earth objects

The Lincoln Near-Earth Asteroid Research (LINEAR) project is a collaboration of the United States Air Force, NASA, and the Massachusetts Institute of Technology's Lincoln Laboratory for the systematic detection and tracking of near-Earth objects. LINEAR was responsible for the majority of asteroid discoveries from 1998 until it was overtaken by the Catalina Sky Survey in 2005. As of 15 September 2011, LINEAR had detected 231,082 new small Solar System bodies, of which at least 2,423 were near-Earth asteroids and 279 were comets. The instruments used by the LINEAR program are located at Lincoln Laboratory's Experimental Test Site (ETS) on the White Sands Missile Range (WSMR) near Socorro, New Mexico.

Near-Earth Asteroid Tracking (NEAT) was a program run by NASA and the Jet Propulsion Laboratory, surveying the sky for near-Earth objects. NEAT was conducted from December 1995 until April 2007, at GEODSS on Hawaii, as well as at Palomar Observatory in California. With the discovery of more than 40 thousand minor planets, NEAT has been one of the most successful programs in this field, comparable to the Catalina Sky Survey, LONEOS and Mount Lemmon Survey.

<span class="mw-page-title-main">1620 Geographos</span> Asteroid

1620 Geographos, provisional designation 1951 RA, is a highly elongated, stony asteroid, near-Earth object and potentially hazardous asteroid of the Apollo group, with a mean-diameter of approximately 2.5 km (1.6 mi). It was discovered on 14 September 1951, by astronomers Albert George Wilson and Rudolph Minkowski at the Palomar Observatory in California, United States. The asteroid was named in honor of the National Geographic Society.

<span class="mw-page-title-main">Spacewatch</span> Astronomical survey that specializes in the study of minor planets

The Spacewatch Project is an astronomical survey that specializes in the study of minor planets, including various types of asteroids and comets at University of Arizona telescopes on Kitt Peak near Tucson, Arizona, in the United States. The Spacewatch Project has been active longer than any other similar currently active programs.

Brian A. Skiff is an American astronomer noted for discovering numerous asteroids and a number of comets including the periodic comets 114P/Wiseman–Skiff and 140P/Bowell–Skiff.

Roy A. Tucker (1951 – 2021) was an American astronomer best known for the co-discovery of near-Earth asteroid 99942 Apophis (formerly known as 2004 MN4) along with David J. Tholen and Fabrizio Bernardi of the University of Hawaii. He was a prolific discoverer of minor planets, credited by the Minor Planet Center with the discovery of 702 numbered minor planets between 1996 and 2010. He also discovered two comets: 328P/LONEOS–Tucker and C/2004 Q1, a Jupiter-family and near-parabolic comet, respectively.

The OCA–DLR Asteroid Survey (ODAS) was an astronomical survey to search for small Solar System bodies focusing on near-Earth objects in the late 1990s. This European scientific project was a collaboration between the French Observatoire de la Côte d'Azur (OCA) and the German Aerospace Center (DLR). The survey is credited for the discovery of one comet and more than 1000 minor planets during 1996–1999.

The Črni Vrh Observatory is an astronomical observatory located in western Slovenia, close to the settlement of Črni Vrh, near the town of Idrija. The current observatory was built in 1985 and stands at an elevation of 730 metres (2,400 ft). Much of the construction was done by volunteers.

<span class="mw-page-title-main">Pan-STARRS</span> Multi-telescope astronomical survey

The Panoramic Survey Telescope and Rapid Response System located at Haleakala Observatory, Hawaii, US, consists of astronomical cameras, telescopes and a computing facility that is surveying the sky for moving or variable objects on a continual basis, and also producing accurate astrometry and photometry of already-detected objects. In January 2019 the second Pan-STARRS data release was announced. At 1.6 petabytes, it is the largest volume of astronomical data ever released.

<span class="mw-page-title-main">1627 Ivar</span>

1627 Ivar, provisional designation 1929 SH, is an elongated stony asteroid and near-Earth object of the Amor group, approximately 15×6×6 km. It was discovered on 25 September 1929, by Danish astronomer Ejnar Hertzsprung at Leiden Southern Station, annex to the Johannesburg Observatory in South Africa. It was named after Ivar Hertzsprung, brother of the discoverer. 1627 Ivar was the first asteroid to be imaged by radar, in July 1985 by the Arecibo Observatory.

James Whitney Young is an American astronomer who worked in the field of asteroid research. After nearly 47 years with the Jet Propulsion Laboratory at their Table Mountain Facility, Young retired July 16, 2009.

<span class="nowrap">(185851) 2000 DP<sub>107</sub></span>

(185851) 2000 DP107 is a sub-kilometer sized asteroid, classified as potentially hazardous asteroid and near-Earth object of the Apollo group that is notable because it provided evidence for binary asteroids in the near-Earth population. The PROCYON probe developed by JAXA and the University of Tokyo was intended to flyby this asteroid before its ion thruster failed and could not be restarted.

4257 Ubasti, provisional designation 1987 QA, is a stony asteroid, classified as near-Earth object of the Apollo group and as Mars-crosser, approximately 1.5 kilometers in diameter. It was discovered by American astronomer Jean Mueller at the Palomar Observatory in California on 23 August 1987. The asteroid was named for Bastet – also known as Baast, Ubaste or Ubasti – the Egyptian goddess of cats.

(101869) 1999 MM is a sub-kilometer asteroid on an eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group. It was discovered on 20 June 1999, by the Lowell Observatory Near-Earth-Object Search (LONEOS) at its U.S. Anderson Mesa Station in Flagstaff, Arizona. The first observation was made by Catalina Sky Survey just 8 days before its official discovery.

<span class="mw-page-title-main">161989 Cacus</span> Near-Earth asteroid in 1941/2022

161989 Cacus is a stony asteroid, classified as near-Earth object and a potentially hazardous asteroid of the Apollo group, approximately 1 kilometer in diameter. It was discovered on 8 February 1978, by German astronomer Hans-Emil Schuster at ESO's La Silla Observatory in northern Chile. Its orbit is confined between Venus and Mars.

(31345) 1998 PG is an eccentric, stony asteroid and binary system, classified as near-Earth object of the Amor group of asteroids, approximately 900 meters in diameter. It minor-planet moon, S/2001 (31345) 1, has an estimated diameter of 270 meters.

(16960) 1998 QS52 (provisional designation 1998 QS52) is a stony asteroid on a highly eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 4.1 kilometers (2.5 mi) in diameter. It was discovered on 25 August 1998, by astronomers of the LINEAR program at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. This asteroid is one of the largest potentially hazardous asteroid known to exist.

<span class="nowrap">(52768) 1998 OR<sub>2</sub></span> Asteroid

(52768) 1998 OR2 (provisional designation 1998 OR2) is an asteroid on an eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Amor group, with a diameter of 2 kilometers (1.2 mi). It was discovered on 24 July 1998, by astronomers of the Near-Earth Asteroid Tracking (NEAT) program at the Haleakala Observatory, Hawaii. It is one of the brightest and therefore largest potentially hazardous asteroids known to exist. With an observation arc of 35 years, the asteroid has a well-determined orbit, and its trajectory is well known through the year 2197. The asteroid's orbit is only potentially hazardous on a time scale of thousands of years.

<span class="mw-page-title-main">2018 AH</span> Near-Earth asteroid Christmas 2021

2018 AH is a sub-kilometer asteroid, classified as near-Earth object of the Apollo group, approximately 100 m (300 ft) in diameter. It was first observed on 4 January 2018, by the Asteroid Terrestrial-impact Last Alert System (ATLAS) on Mauna Loa and quickly followed-up by many other surveys, with precovery observations found from Pan-STARRS and PTF from the day previous.

2020 SL1 is a near-Earth asteroid of the Apollo group, discovered by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii on 18 September 2020. With an estimated diameter of 0.9–2.0 km (0.56–1.24 mi), it is the largest potentially hazardous asteroid discovered in 2020.

References

  1. 1 2 3 "Minor Planet Discoverers (by number)". Minor Planet Center. 10 July 2017. Retrieved 5 October 2017.
  2. "USNO Image and Catalogue Archive". Archived from the original on 2017-11-04. Retrieved 2008-03-02.
  3. CMC14
  4. Yahoo Groups
  5. Summary of PHA and NEA Discoveries by Discoverers
  6. "NEODyS".
  7. MPEC 1999-H17 : 1999 HF1
  8. NASA Snaps Pics Of 'Space Peanut' As It Passes By Earth, Ted Ranosa, Tech Times, 3 August 2015.
  9. MPEC 1999-X19 : 1999 XS35
  10. MPEC 2001-P40 : 2001 OG108
  11. "JPL Close-Approach Data: 153814 (2001 WN5)" (2011-01-04 last obs (arc=14.9 years)). Retrieved 2011-10-16.
  12. MPEC 2003-T03 : 2003 SQ222
  13. MPEC 2003-T74 : 1937 UB (HERMES)
  14. MPEC 2004-J60 : 2004 JG6