Robert H. McNaught

Last updated

Minor planets discovered: 483 [1]
see § List of discovered minor planets

Robert H. McNaught (born in Scotland[ citation needed ] in 1956[ citation needed ]) is a Scottish-Australian astronomer at the Research School of Astronomy and Astrophysics of the Australian National University (ANU).[ citation needed ] He has collaborated with David J. Asher of the Armagh Observatory.[ citation needed ]

Contents

The inner main-belt asteroid 3173 McNaught, discovered by Edward Bowell at Anderson Mesa Station in 1981, was named after him by its discoverer, following a suggestion by David Seargent. [2]

Work

McNaught is a prolific discoverer of asteroids and comets, described as "the world's greatest comet discoverer" [3] and he participated in the Siding Spring Survey (SSS) using the ANU's Uppsala Southern Schmidt Telescope. [4] He discovered the Great Comet C/2006 P1 on 7 August 2006, the brightest comet in several decades, which became easily visible to the naked eye for observers in the Southern Hemisphere. [5] The SSS was the only active professional Near Earth Object survey in the Southern Hemisphere. The survey ended in 2013 after funding dried up. [6]

McNaught previously worked on the Anglo-Australian Near-Earth Asteroid Survey from 1990 to 1996. [7]

Other work

McNaught worked at the University of Aston's satellite-tracking camera originally outside Evesham in 1982, thereafter at Herstmonceux and more recently at Siding Spring. In his spare time he successfully conducts patrols for novae, identifies images of prenovae and unusual variable stars on survey plates, measures their positions, makes astrometric observations of comets and minor planets and photometric observations of comets and novae. He also carries out extensive observational and computational work on meteors, as well as on occultations by minor planets.

Funding issues

In October 2011, partly due to changes in the exchange rate between the Australian and US dollars, Catalina Sky Survey of NASA had to end funding McNaught's southern survey, [8] which used to cost $110,000 per year, [9] ending the international cooperation in July 2012. The astronomer estimated that the survey needs $180,000 annually, plus a small one-time sum to fix the observatory dome. [8] For several months the project was temporarily funded from the ANU, but in late 2012, the ANU advised that it could no longer support the program and that funds would not be available from January 2013. [10] [ failed verification ]

Discoveries

List of cometary discoveries

In total, McNaught has discovered 82 comets.

Long-period

McNaught has discovered 44 long-period comets:

  • C/1987 U3 (a. k. a. 1987 XXXII, 1987b1)
  • C/2005 E2
  • C/2005 L2
  • C/2005 L3
  • C/2005 S4
  • C/2006 B1
  • C/2006 E1
  • C/2006 K1
  • C/2006 K3
  • C/2006 L2
  • C/2006 P1 (Great Comet of 2007)
  • C/2006 Q1
  • C/2007 K6
  • C/2007 M1
  • C/2007 P1
  • C/2007 T1
  • C/2007 Y2
  • C/2008 A1
  • C/2008 J4
  • C/2009 F2
  • C/2009 F4
  • C/2009 F5
  • C/2009 K5
  • C/2009 R1
  • C/2009 T1
  • C/2010 J2
  • C/2011 C1
  • C/2011 G1
  • C/2011 L2
  • C/2011 L3
  • C/2011 N2
  • C/2011 Q2
  • C/2011 R1
  • C/2012 C1
  • C/2012 H2
  • C/2012 K6
  • C/2012 T4
  • C/2012 Y3
  • C/2013 A1
  • C/2013 E1
  • C/2013 F3
  • C/2013 G2
  • C/2013 G7
  • C/2013 J3
  • C/2013 O3

Short period

McNaught has discovered 26 short-period comets:

  • 191P/McNaught
  • 220P/McNaught
  • 254P/McNaught
  • 260P/McNaught
  • 278P/McNaught
  • P/2004 R1 (McNaught)
  • P/2005 J1 (McNaught)
  • P/2005 L1 (McNaught)
  • P/2005 Y2 (McNaught)
  • P/2006 G1 (McNaught)
  • P/2006 H1 (McNaught)
  • P/2007 H1 (McNaught)
  • P/2008 J3 (McNaught)
  • P/2008 O2 (McNaught)
  • P/2008 Y3 (McNaught)
  • P/2009 Q5 (McNaught)
  • P/2009 S2 (McNaught)
  • P/2009 U4 (McNaught)
  • P/2010 J5 (McNaught)
  • P/2011 L1 (McNaught)
  • P/2011 P1 (McNaught)
  • P/2011 Q3 (McNaught)
  • P/2012 O1 (McNaught)
  • P/2012 O2 (McNaught)
  • P/2012 O3 (McNaught)
  • P/2013 J2 (McNaught)

Co-discoveries

McNaught is the co-discoverer of the following comets:

  • P/Catalina-McNaught (a.k.a. P/2008 S1, 2008 JK)
  • P/McNaught-Hartley (a.k.a. P/1994 N2, 1994 XXXI, 1994n)
  • Comet McNaught-Hartley (a.k.a. C/1999 T1)
  • Comet McNaught-Tritton (a.k.a. C/1978 G2, 1978 XXVII)
  • Comet McNaught-Watson (a.k.a. C/1999 S2)

Groups

Comets McNaught-Hughes
Comets McNaught-Russell
  • C/1991 C3 (a.k.a. 1990 XIX, 1991g)
  • C/1991 Q1 (a.k.a. 1992 XI, 1991v)
  • C/1991 R1 (a.k.a. 1990 XXII, 1991w)
  • C/1993 Y1 (a.k.a. 1994 XI, 1993v)
  • 262P/McNaught-Russell (a.k.a. 1994 XXIV, 1994u)

List of discovered minor planets

As of 2016, Robert McNaught is credited by the Minor Planet Center with the discovery and co-discovery of 483 minor planets during 1975–2005. [1]

3904 Honda22 February 1988 list
4093 Bennett4 November 1986 list
4128 UKSTU28 January 1988 list
4129 Richelen22 February 1988 list
4220 Flood22 February 1988 list
4456 Mawson27 July 1989 list
4499 Davidallen4 January 1989 list
4504 Jenkinson21 December 1989 list
4638 Estens2 March 1989 list
4667 Robbiesh4 November 1986 list
4678 Ninian24 September 1990 list
4679 Sybil9 October 1990 list
4699 Sootan4 November 1986 list
4704 Sheena28 January 1988 list
4710 Wade4 January 1989 list
4713 Steel 26 August 1989 list
(4953) 1990 MU 23 June 1990 list
4956 Noymer12 November 1990 list
4974 Elford14 June 1990 list
5007 Keay20 October 1990 list
5061 McIntosh22 February 1988 list
5066 Garradd22 June 1990 list
5068 Cragg9 October 1990 list
5133 Phillipadams12 August 1990 list
5136 Baggaley20 October 1990 list
(5189) 1990 UQ20 October 1990 list
5277 Brisbane22 February 1988 list
5329 Decaro21 December 1989 list
5335 Damocles 18 February 1991 list
5378 Ellyett9 April 1991 list
5380 Sprigg 7 May 1991 list
5382 McKay8 May 1991 list
5441 Andymurray8 May 1991 list
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5475 Hanskennedy 26 August 1989 list
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5691 Fredwatson26 March 1992 list
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5782 Akirafujiwara7 January 1991 list
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5883 Josephblack6 November 1993 list
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7170 Livesey30 June 1987 list
7177 Melvyntaylor9 October 1990 list
7247 Robertstirling12 October 1991 list
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8115 Sakabe24 April 1996 list [B]
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(9899) 1996 EH12 March 1996 list
9984 Gregbryant18 April 1996 list [D]
9985 Akiko12 May 1996 list [A]
10058 Ikwilliamson25 February 1988 list
(10098) 1991 SC130 September 1991 list
10188 Yasuoyoneda14 May 1996 list [B]
(10342) 1991 TQ1 October 1991 list
(10511) 1989 OD21 July 1989 list
(10525) 1990 TO12 October 1990 list
10736 Marybrück22 February 1988 list
10737 Brück25 February 1988 list
10773 Jamespaton7 January 1991 list
10841 Ericforbes12 August 1994 list
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12446 Juliabryant15 August 1996 list [D]
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12819 Susumutakahasi12 May 1996 list [B]
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(13060) 1991 EJ10 March 1991 list
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13176 Kobedaitenken21 April 1996 list [A]
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(322074) 2010 VB11213 April 2004 list
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(382395) 1990 SM22 September 1990 list [E]
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(455172) 1999 QJ17 August 1999 list
(480808) 1994 XL1 6 December 1994 list
(480825) 1999 PL13 August 1999 list
Co-discovery made with:
A H. Abe
B Y. Ikari
C T. Kojima
D J. B. Child
E P. McKenzie

List of novae

See also

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Ingrid van Houten-Groeneveld was a Dutch astronomer.

Andrea Boattini is an Italian astronomer and a prolific discoverer of minor planets and comets.

Francesco Manca is an Italian amateur astronomer and discoverer of minor planets at the Sormano Astronomical Observatory in northern Italy.

<span class="mw-page-title-main">Siding Spring Observatory</span> Astronomic observatory in New South Wales, Australia

Siding Spring Observatory near Coonabarabran, New South Wales, Australia, part of the Research School of Astronomy & Astrophysics (RSAA) at the Australian National University (ANU), incorporates the Anglo-Australian Telescope along with a collection of other telescopes owned by the Australian National University, the University of New South Wales, and other institutions. The observatory is situated 1,165 metres (3,822 ft) above sea level in the Warrumbungle National Park on Mount Woorat, also known as Siding Spring Mountain. Siding Spring Observatory is owned by the Australian National University (ANU) and is part of the Mount Stromlo and Siding Spring Observatories research school.

<span class="mw-page-title-main">Orbital eccentricity</span> Amount by which an orbit deviates from a perfect circle

In astrodynamics, the orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greater than 1 is a hyperbola. The term derives its name from the parameters of conic sections, as every Kepler orbit is a conic section. It is normally used for the isolated two-body problem, but extensions exist for objects following a rosette orbit through the Galaxy.

<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">Siding Spring Survey</span> Observatory

The Siding Spring Survey (SSS) was a near-Earth object search program that used the 0.5-metre Uppsala Southern Schmidt Telescope at Siding Spring Observatory, New South Wales, Australia. It was the southern hemisphere counterpart of the Catalina Sky Survey (CSS) located in the Santa Catalina Mountains on Mount Bigelow, near Tucson, Arizona, USA. The survey was the only professional search for dangerous asteroids being made in the Southern Hemisphere.

<span class="mw-page-title-main">La Cañada Observatory</span> Observatory

La Cañada Observatory, is an astronomical observatory in Ávila, Spain privately owned by Juan Lacruz, the main activity is to monitor near-Earth objects other asteroids and comets.

<span class="mw-page-title-main">C/2006 M4 (SWAN)</span>

Comet C/2006 M4 (SWAN) is a non-periodic comet discovered in late June 2006 by Robert D. Matson of Irvine, California and Michael Mattiazzo of Adelaide, South Australia in publicly available images of the Solar and Heliospheric Observatory (SOHO). These images were captured by the Solar Wind ANisotropies (SWAN) Lyman-alpha all-sky camera on board the SOHO. The comet was officially announced after a ground-based confirmation by Robert McNaught on July 12.

<span class="mw-page-title-main">Comet McNaught</span> Non-periodic comet

Comet McNaught, also known as the Great Comet of 2007 and given the designation C/2006 P1, is a non-periodic comet discovered on 7 August 2006 by British-Australian astronomer Robert H. McNaught using the Uppsala Southern Schmidt Telescope. It was the brightest comet in over 40 years, and was easily visible to the naked eye for observers in the Southern Hemisphere in January and February 2007.

Comet McNaught can refer to any one of more than 50 comets discovered by the astronomer Robert H. McNaught.

The Uppsala Schmidt Telescope is a Schmidt telescope located in Australia. It was moved to Siding Spring Observatory from Mount Stromlo Observatory in 1982. The instrument has been used to study galaxies, asteroids and comets. It was last dedicated to the Siding Spring Survey. The telescope had a field of view of just over 6° through the use of a correcting plate, making its field three times as large as that of the Anglo-Australian Telescope. It used a spherical rather than a parabolic mirror with 0.6 m correcting plate to achieve this. Photographic plates and film were used as detectors.

<span class="mw-page-title-main">Comet tail</span> Dust or gases blown off a comet by solar wind in the inner solar system, leaving a visible trail

A comet tail and coma are visible features of a comet when they are illuminated by the Sun and may become visible from Earth when a comet passes through the inner Solar System. As a comet approaches the inner Solar System, solar radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them.

<span class="mw-page-title-main">C/2009 R1 (McNaught)</span> Non-periodic comet discovered in 2009

C/2009 R1 (McNaught), one of more than fifty comets known as Comet McNaught, is a non-periodic comet discovered by British-Australian astronomer Robert H. McNaught on September 9, 2009, using the Uppsala Southern Schmidt Telescope at Siding Spring Observatory in New South Wales, Australia. The discovery was confirmed the same day at the Optical Ground Station telescope at Tenerife. After the discovery, earlier images of the comet were found from July 20, August 1, and August 18, 2009. It is believed that C/2009 R1 has left the Solar System permanently.

The Edgar Wilson Award is an annual international award established in 1998 consisting of a monetary award and a plaque allocated annually to amateur comet discoverers. It is administered by the Smithsonian Astrophysical Observatory (SAO) through the IAU's Central Bureau for Astronomical Telegrams (CBAT).

<span class="mw-page-title-main">Astronomical Society of New South Wales</span> Amateur astronomy club in the state of New South Wales, Australia

The Astronomical Society of New South Wales (ASNSW) is an amateur astronomy club in the state of New South Wales, Australia, founded in 1954.

P/2011 P1 (McNaught) was a Jupiter-family comet that passed extremely close to Jupiter on 4 December 2010 and disintegrated by 2012. It was discovered on 1 August 2011 by astronomer Robert H. McNaught at the Siding Spring Observatory in New South Wales, Australia. With an observation arc of 415 days, the comet's nominal orbit solution suggests that its 2010 approach distance was 0.00084 astronomical units from Jupiter's center—well within Jupiter's Roche limit at which the comet would be torn apart by tidal forces. The earliest precovery image of the comet was taken by Pan-STARRS 1 on 6 December 2010, two days after the comet's close pass with Jupiter.

References

  1. 1 2 "Minor Planet Discoverers (by number)". Minor Planet Center. 22 August 2016. Retrieved 24 August 2016.
  2. Schmadel, Lutz D. (2007). "(3173) McNaught". Dictionary of Minor Planet Names – (3173) McNaught. Springer Berlin Heidelberg. p. 263. doi:10.1007/978-3-540-29925-7_3174. ISBN   978-3-540-00238-3.
  3. Mobberley, Martin (2011). Hunting and imaging comets. New York: Springer. p. 75. ISBN   9781441969057.
  4. "Earth-threatening space rocks hunted by ANU". Media releases. Australian National University. 6 April 2004. Retrieved 21 January 2007.
  5. Kronk, Gary. "C/2007 P1 (McNaught)". Cometography. Retrieved 24 April 2013.
  6. Safi, Michael (20 October 2014). "Earth at risk after cuts close comet-spotting program, scientists warn". The Guardian . Retrieved 25 November 2015.
  7. "AANEAS". Mt Stromlo Observatory. Archived from the original on 29 February 2016. Retrieved 27 November 2015.
  8. 1 2 "Vital eye for killer asteroids could shut imminently".
  9. "Comet century may be telescope's last › News in Science (ABC Science)". Australian Broadcasting Corporation . 14 May 2013.
  10. Vlahos, Perry (20 December 2012). "Who's on night watch?". Sydney Morning Herald.