115P/Maury

Last updated
115P/Maury
115P 2020-07-27 image ZTF-sso-436-zr-fov-3.5 arcmin.png
Discovery
Discovered by Alain Maury
Discovery dateAugust 16, 1985
Orbital characteristics
Epoch March 13, 2013 (2456364.5) [1]
Aphelion 6.4797164 AU
Perihelion 2.0396989 AU
Semi-major axis 4.259707 AU
Eccentricity 0.52116457
Orbital period 8.79 a
3211.205 d
Inclination 11.687384°
Last perihelion2020-Jul-29 [2]
Next perihelion2029-May-18 [3]

115P/Maury, is a periodic Jupiter-family comet, discovered on August 16, 1985, from the Palomar Observatory by Alain Maury. When the comet was first announced on 1985 September 6, the confirmation came quickly from other observers located at the Palomar Observatory. To the initial announcement of the comet, several confirmations were announced in multiple different reports were compiled by S. Singer-Brewster, D. Schneeberger, and M. Gallup that found the 15th-magnitude trail of the comet on a plate exposed with the 0.46-m Schmidt telescope. These came from the staff at Palomar Observatory, who used the 1.5-m reflector and a CCD to detect the comet. The comet was continued to be followed and detected, leading to Scientist giving the comet a 8.6 to 8.8 orbital period. [4]

The nucleus of the comet has a radius of about 1.1 kilometers based on observations by Keck, assuming a geometric albedo of 0.04. [5]

Related Research Articles

<span class="mw-page-title-main">Halley's Comet</span> Short-period comet visible every 75–76 years

Halley's Comet, Comet Halley, or sometimes simply Halley, officially designated 1P/Halley, is a short-period comet visible from Earth every 75–79 years. Halley is the only known short-period comet that is regularly visible to the naked eye from Earth, and thus the only naked-eye comet that can appear twice in a human lifetime. It last appeared in the inner parts of the Solar System in 1986 and will next appear in mid-2061.

<span class="mw-page-title-main">2060 Chiron</span> Large 200km centaur/comet with 50-year orbit

2060 Chiron is a small Solar System body in the outer Solar System, orbiting the Sun between Saturn and Uranus. Discovered in 1977 by Charles Kowal, it was the first-identified member of a new class of objects now known as centaurs—bodies orbiting between the asteroid belt and the Kuiper belt.

<span class="mw-page-title-main">29P/Schwassmann–Wachmann</span> Periodic comet with 14 year orbit

Comet 29P/Schwassmann–Wachmann, also known as Schwassmann–Wachmann 1, was discovered on November 15, 1927, by Arnold Schwassmann and Arno Arthur Wachmann at the Hamburg Observatory in Bergedorf, Germany. It was discovered photographically, when the comet was in outburst and the magnitude was about 13. Precovery images of the comet from March 4, 1902, were found in 1931 and showed the comet at 12th magnitude.

<span class="mw-page-title-main">Comet Encke</span> Periodic comet with 3-year orbit

Comet Encke, or Encke's Comet, is a periodic comet that completes an orbit of the Sun once every 3.3 years. Encke was first recorded by Pierre Méchain on 17 January 1786, but it was not recognized as a periodic comet until 1819 when its orbit was computed by Johann Franz Encke. Like Halley's Comet, it is unusual in its being named after the calculator of its orbit rather than its discoverer. Like most comets, it has a very low albedo, reflecting only 4.6% of the light its nucleus receives, although comets generate a large coma and tail that can make them much more visible during their perihelion. The diameter of the nucleus of Encke's Comet is 4.8 km.

<span class="mw-page-title-main">Tempel 1</span> Jupiter-family comet

Tempel 1 is a periodic Jupiter-family comet discovered by Wilhelm Tempel in 1867. It completes an orbit of the Sun every 5.6 years. Tempel 1 was the target of the Deep Impact space mission, which photographed a deliberate high-speed impact upon the comet in 2005. It was re-visited by the Stardust spacecraft on February 14, 2011, and came back to perihelion in August 2016. On 26 May 2024, it will make a modest approach of 0.55 AU to Jupiter which will lift the perihelion distance and 9P will next come to perihelion on 12 February 2028 when it will be 1.77 AU from the Sun.

<span class="mw-page-title-main">4P/Faye</span> Periodic comet with 7 year orbit

Comet 4P/Faye is a periodic Jupiter-family comet discovered in November 1843 by Hervé Faye at the Royal Observatory in Paris. Its most recent perihelia were on November 15, 2006; May 29, 2014; and September 8, 2021.

<span class="mw-page-title-main">53P/Van Biesbroeck</span> Periodic comet with 12 year orbit

53P/Van Biesbroeck is a periodic comet 7 km in diameter. Its current orbital period is 12.53 years.

56P/Slaughter–Burnham is a periodic comet in the Solar System with a period of 11.54 years.

71P/Clark is a periodic comet in the Solar System with an orbital period of 5.5 years.

<span class="mw-page-title-main">73P/Schwassmann–Wachmann</span> Multiple fragment periodic comet with 5-year orbit

73P/Schwassmann–Wachmann, also known as Schwassmann–Wachmann 3 or SW3 for short, is a periodic comet that has a 5.4 year orbital period and that has been actively disintegrating since 1995. When it came to perihelion in March 2017, fragment 73P-BT was separating from the main fragment 73P-C. Fragments 73P-BU and 73P-BV were detected in July 2022. The main comet came to perihelion on 25 August 2022, when the comet was 0.97 AU from the Sun and 1 AU from Earth. It will be less than 80 degrees from the Sun from 25 May 2022 until August 2023. On 3 April 2025 it will make a modest approach of 0.3 AU to Jupiter. 73P will next come to perihelion on 23 December 2027 when it will be 0.92 AU from the Sun and on the far side of the Sun 1.9 AU from Earth.

<span class="mw-page-title-main">114P/Wiseman–Skiff</span> Periodic comet with 6 year orbit

114P/Wiseman–Skiff is a periodic comet in the Solar System.

<span class="mw-page-title-main">15P/Finlay</span> Periodic comet with 6 year orbit

Comet Finlay is a periodic comet with an orbital period of 6 years discovered by William Henry Finlay on September 26, 1886. The next perihelion passage is July 13, 2021 when the comet will have a solar elongation of 54 degrees at approximately apparent magnitude 10. It last came to perihelion on December 27, 2014, at around magnitude 10. Of the numbered periodic comets, the orbit of 15P/Finlay has one of the smallest minimum orbit intersection distances with the orbit of Earth (E-MOID). In October 2060 the comet will pass about 5 million km from Earth.

<span class="mw-page-title-main">24P/Schaumasse</span> Periodic comet with 8 year orbit

Comet Schaumasse is a periodic comet discovered by Alexandre Schaumasse on 1 December 1911 as 12th magnitude. It next comes to perihelion on 8 January 2026 and should brighten to about magnitude 9.

<span class="mw-page-title-main">45P/Honda–Mrkos–Pajdušáková</span> Periodic comet with 5 year orbit

45P/Honda–Mrkos–Pajdušáková is a short-period comet discovered by Minoru Honda December 3, 1948. It is named after Minoru Honda, Antonín Mrkos, and Ľudmila Pajdušáková. The object revolves around the Sun on an elliptical orbit with a period of 5.25 years. The nucleus is 1.3 kilometers in diameter. On August 19 and 20, 2011, it became the fifteenth comet detected by ground radar telescope.

<span class="mw-page-title-main">50P/Arend</span> Periodic comet with 8 year orbit

Comet Arend or 50P/Arend is a periodic comet in the Solar System which was discovered on October 4, 1951. It was discovered by astronomer Sylvain Julien Victor Arend at the Royal Observatory of Belgium located in the municipality of Uccle. The comet was illustrated at approximately a magnitude of 14 and also exhibited a nucleus within a coma 14 arc seconds across. From its discovery, the comet has had 7 perihelions with its last return of Earth recorded on November 1, 2007. The comet's next perihelion will be in the year 2024.

C/2001 OG108 (LONEOS) is a Halley-type comet with an orbital period of 48.51 years. It was discovered on 28 July 2001 by the LONEOS telescope at Lowell Observatory. Of the short-period comets with known diameters and perihelion inside the orbit of Earth, C/2001 OG108 is the second largest after Comet Swift–Tuttle.

<span class="mw-page-title-main">276P/Vorobjov</span>

276P/Vorobjov is a Jupiter-family comet discovered on 15 October 2012 by Tomáš Vorobjov on three 120-s images taken remotely using the 0.81-m f/7 Ritchey-Chretien Schulman Telescope located at the Mt. Lemmon SkyCenter via the Sierra Stars Observatory Network in the course of a minor-planet search survey undertaken as part of the International Astronomical Search Collaboration (IASC) school campaigns. After posting on the Minor Planet Center's NEOCP webpage, other observers have commented on the object's cometary appearance. The discovery was announced by the Minor Planet Center on 18 October, three days after the discovery.

51P/Harrington is a periodic comet in the Solar System.

92P/Sanguin, also called Sanguin's Comet or Comet Sanguin, is a Jupiter-family comet discovered on October 15, 1977, by Juan G. Sanguin at Leoncito Astronomical Complex. It completes a single rotation approximately every 6 days.

<span class="nowrap">C/2014 UN<sub>271</sub></span> (Bernardinelli–Bernstein) Largest known Oort cloud comet

C/2014 UN271 (Bernardinelli–Bernstein), simply known as C/2014 UN271 or Comet Bernardinelli–Bernstein (nicknamed BB), is a large Oort cloud comet discovered by astronomers Pedro Bernardinelli and Gary Bernstein in archival images from the Dark Energy Survey. When first imaged in October 2014, the object was 29 AU (4.3 billion km; 2.7 billion mi) from the Sun, almost as far as Neptune's orbit and the greatest distance at which a comet has been discovered. With a nucleus diameter of at least 120 km (75 mi), it is the largest Oort cloud comet known. It is approaching the Sun and will reach its perihelion of 10.9 AU (just outside of Saturn's orbit) in January 2031. It will not be visible to the naked eye because it will not enter the inner Solar System.

References

  1. Jet Propulsion Laboratory. "115P/Maury" . Retrieved 2013-06-02.
  2. "115P/Maury Orbit". Minor Planet Center . Retrieved 2014-06-17.
  3. "Horizons Batch for 115P/Maury (90000993) on 2029-May-18" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons . Retrieved 2023-07-06. (JPL#43 Soln.date: 2023-May-03)
  4. "115P/Maury". cometography.com. Retrieved 2019-08-01.
  5. Meech, K.J.; Hainaut, O.R.; Marsden, B.G. (August 2004). "Comet nucleus size distributions from HST and Keck telescopes". Icarus. 170 (2): 463–491. Bibcode:2004Icar..170..463M. doi:10.1016/j.icarus.2004.03.014.
Numbered comets
Previous
114P/Wiseman–Skiff
115P/MauryNext
116P/Wild