2009 Jupiter impact event

Last updated

2009 Jupiter impact event
Hs-2009-23-crop.jpg
Hubble image of the scar taken on July 23 showing a blemish of about 8,000 kilometres (5,000 mi) long [1] [2]
DateJuly 19, 2009 (2009-07-19)
Location Jupiter
A picture of the 2009 impact mark captured by NASA Infrared Telescope Facility in Mauna Kea, Hawaii Jupiter impact jul2009.jpg
A picture of the 2009 impact mark captured by NASA Infrared Telescope Facility in Mauna Kea, Hawaii
Keck Observatory (the two in the middle) and NASA Infrared Telescope Facility (right) at Mauna Kea, Hawaii The Keck Subaru and Infrared obervatories.JPG
Keck Observatory (the two in the middle) and NASA Infrared Telescope Facility (right) at Mauna Kea, Hawaii

The 2009 Jupiter impact event, occasionally referred to as the Wesley impact, was a July 2009 impact event on Jupiter that caused a black spot in the planet's atmosphere. The impact area covered 190 million square kilometers, similar in area to the planet's Little Red Spot and approximately the size of the Pacific Ocean. [3] The impactor is estimated to have been about 200 to 500 meters in diameter. [4] (For comparison, the one for the Tunguska event was estimated to be in the 60–190 meters range.)

Contents

Discovery

Amateur astronomer Anthony Wesley discovered the impact at approximately 13:30 UTC on 19 July 2009 (exactly 15 years after the Jupiter impacts of comet Shoemaker–Levy 9, or SL9). He was at his home observatory just outside Murrumbateman, New South Wales, Australia, using stacked images on a 14.5-inch (36.8 cm) diameter reflecting telescope equipped with a low light machine vision video camera attached to the telescope. [5] Wesley stated that:

When first seen close to the limb (and in poor conditions) it was only a vaguely dark spot, I [thought] likely to be just a normal dark polar storm. However as it rotated further into view, and the conditions improved I suddenly realised that it wasn't just dark, it was black in all channels, meaning it was truly a black spot. [6]

Wesley sent an e-mail to others including the NASA Jet Propulsion Laboratory in Pasadena, California reporting his observations. [7]

Findings

Paul Kalas and collaborators confirmed the sighting. They had time on the Keck II telescope in Hawaii, and had been planning to observe Fomalhaut b, but they spent some of their time looking at the Jupiter impact. [8] Infrared observation by Keck and the NASA Infrared Telescope Facility (IRTF) [3] at Mauna Kea showed a bright spot where the impact took place, indicating the impact warmed a 190 million square km area of the lower atmosphere at 305° west, 57° south near Jupiter's south pole. [3]

The spot's prominence indicated that it was composed of high-altitude aerosols similar to those seen during the SL9 impact. [8] Using near-infrared wavelengths and the IRTF, Glenn Orton and his team detected bright upwelling particles in the planet's upper atmosphere and using mid-infrared wavelengths, found possible extra emission of ammonia gas. [9]

The force of the explosion on Jupiter was thousands of times more powerful than the suspected comet or asteroid that exploded over the Tunguska River Valley in Siberia in June 1908. [2] (This would be approximately 12,500–13,000 megatons of TNT, over a million times more powerful than the bomb dropped on Hiroshima). [10]

Impactor

The object that hit Jupiter was not identified before Wesley discovered the impact. A 2003 paper estimated comets with a diameter larger than 1.5 kilometers impact Jupiter about every 90 to 500 years, [11] while a 1997 survey suggested that the astronomer Cassini may have recorded an impact in 1690. [12]

Given the size of the SL9 impactors, [13] it is likely that this object was less than one kilometer in diameter. [2] [14] Finding water at the site would indicate that the impactor was a comet, [15] as opposed to an asteroid or a very small, icy moon. [16] At first it was believed that the object was more likely to be a comet since comets generally have more planet-crossing orbits. [17] At the distance of Jupiter (5.2 AU) most small comets are not close enough to the Sun to be very active, and so would be hard to detect. [17] Small kilometer-sized asteroids would also be hard to detect, however, and recent work by Orton et al. and Hammel et al. has strongly suggested the impactor was an asteroid, as it left only one impact site, did not reduce Jovian decametric radiation emission by contributing significant dust to the Jovian magnetosphere, and produced high altitude dusty debris full of silica, very different than what was produced by SL9.[ citation needed ]

As of 2012, the impactor is believed to have been an asteroid with a diameter of about 200 to 500 meters. [4]

Visibility

Assuming it was an inactive comet (or asteroid) about 1 km in diameter, this object would have been no brighter than about apparent magnitude 25. [17] (Jupiter shines about 130 billion times brighter than a 25th magnitude object.) [18] Most asteroid surveys that use a wide field of view do not see fainter than about magnitude 22 (which is 16x brighter than magnitude 25). [17] Even detecting satellites less than 10 km in diameter orbiting Jupiter is difficult and requires some of the best telescopes in the world. [19] It is only since 1999 with the discovery of Callirrhoe that astronomers have been able to discover many of Jupiter's smallest moons. [20]

See also

Related Research Articles

<span class="mw-page-title-main">Asteroid</span> Minor planets found within the inner Solar System

An asteroid is a minor planet—an object that is neither a true planet nor an identified comet— that orbits within the inner Solar System. They are rocky, metallic, or icy bodies with no atmosphere, classified as C-type (carbonaceous), M-type (metallic), or S-type (silicaceous). The size and shape of asteroids vary significantly, ranging from small rubble piles under a kilometer across and larger than meteoroids, to Ceres, a dwarf planet almost 1000 km in diameter. A body is classified as a comet, not an asteroid, if it shows a coma (tail) when warmed by solar radiation, although recent observations suggest a continuum between these types of bodies.

Comet Shoemaker–Levy 9 was a comet that broke apart in July 1992 and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its possible role in reducing space debris in the inner Solar System.

<span class="mw-page-title-main">Near-Earth object</span> Small Solar System body with an orbit that can bring it close to Earth

A near-Earth object (NEO) is any small Solar System body orbiting the Sun whose closest approach to the Sun (perihelion) is less than 1.3 times the Earth–Sun distance. This definition applies to the object's orbit around the Sun, rather than its current position, thus an object with such an orbit is considered an NEO even at times when it is far from making a close approach of Earth. If an NEO's orbit crosses the Earth's orbit, and the object is larger than 140 meters (460 ft) across, it is considered a potentially hazardous object (PHO). Most known PHOs and NEOs are asteroids, but about 0.35% are comets.

<span class="mw-page-title-main">Impact event</span> Collision of two astronomical objects

An impact event is a collision between astronomical objects causing measurable effects. Impact events have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, as the impacting body is usually traveling at several kilometres a second, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.

<span class="mw-page-title-main">Asteroid impact avoidance</span> Methods to prevent destructive asteroid hits

Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted away, preventing destructive impact events. An impact by a sufficiently large asteroid or other NEOs would cause, depending on its impact location, massive tsunamis or multiple firestorms, and an impact winter caused by the sunlight-blocking effect of large quantities of pulverized rock dust and other debris placed into the stratosphere. A collision 66 million years ago between the Earth and an object approximately 10 kilometers wide is thought to have produced the Chicxulub crater and triggered the Cretaceous–Paleogene extinction event that is understood by the scientific community to have caused the extinction of all non-avian dinosaurs.

<span class="mw-page-title-main">Spaceguard</span> Efforts to study asteroids that might impact Earth

The term Spaceguard loosely refers to a number of efforts to discover, catalogue, and study near-Earth objects (NEO), especially those that may impact Earth.

<span class="mw-page-title-main">Bolide</span> Extremely bright meteor

A bolide is normally taken to mean an exceptionally bright meteor, but the term is subject to more than one definition, according to context. It may refer to any large crater-forming body, or to one that explodes in the atmosphere. It can be a synonym for a fireball, sometimes specific to those with an apparent magnitude of −4 or brighter.

<span class="mw-page-title-main">617 Patroclus</span> Jupiter trojan asteroid

617 Patroclus is a large binary Jupiter trojan asteroid. It is a dark D-type asteroid and a slow rotator, due to the 103-hour orbital period of its two components. It is one of five Jupiter trojan asteroids targeted by the Lucy space probe, and is scheduled for a flyby in 2033.

<span class="mw-page-title-main">Wide-field Infrared Survey Explorer</span> NASA satellite of the Explorer program

Wide-field Infrared Survey Explorer was a NASA infrared astronomy space telescope in the Explorers Program launched in December 2009. WISE discovered thousands of minor planets and numerous star clusters. Its observations also supported the discovery of the first Y-type brown dwarf and Earth trojan asteroid. WISE performed an all-sky astronomical survey with images in 3.4, 4.6, 12 and 22 μm wavelength range bands, over ten months using a 40 cm (16 in) diameter infrared telescope in Earth orbit.

2007 WD5 is an Apollo asteroid some 50 m (160 ft) in diameter and a Mars-crosser asteroid first observed on 20 November 2007, by Andrea Boattini of the Catalina Sky Survey. Early observations of 2007 WD5 caused excitement amongst the scientific community when it was estimated as having as high as a 1 in 25 chance of colliding with Mars on 30 January 2008. However, by 9 January 2008, additional observations allowed NASA's Near Earth Object Program (NEOP) to reduce the uncertainty region resulting in only a 1-in-10,000 chance of impact. 2007 WD5 most likely passed Mars at a distance of 6.5 Mars radii. Due to this relatively small distance and the uncertainty level of the prior observations, the gravitational effects of Mars on its trajectory are unknown and, according to Steven Chesley of NASA's Jet Propulsion Laboratory Near-Earth Object program, 2007 WD5 is currently considered 'lost' (see lost asteroids).

<span class="mw-page-title-main">Potentially hazardous object</span> Hazardous near-Earth asteroid or comet

A potentially hazardous object (PHO) is a near-Earth object – either an asteroid or a comet – with an orbit that can make close approaches to the Earth and which is large enough to cause significant regional damage in the event of impact. They are conventionally defined as having a minimum orbit intersection distance with Earth of less than 0.05 astronomical units and an absolute magnitude of 22 or brighter, the latter of which roughly corresponds to a size larger than 140 meters. More than 99% of the known potentially hazardous objects are no impact threat over the next 100 years. As of September 2022, just 17 of the known potentially hazardous objects listed on the Sentry Risk Table could not be excluded as potential threats over the next hundred years. Over hundreds if not thousands of years though, the orbits of some "potentially hazardous" asteroids can evolve to live up to their namesake.

<span class="mw-page-title-main">NEO Surveyor</span> Space-based infrared telescope

NEO Surveyor, formerly called Near-Earth Object Camera (NEOCam), then NEO Surveillance Mission, is a planned space-based infrared telescope designed to survey the Solar System for potentially hazardous asteroids.

The Asteroid Terrestrial-impact Last Alert System (ATLAS) is a robotic astronomical survey and early warning system optimized for detecting smaller near-Earth objects a few weeks to days before they impact Earth.

Anthony Wesley is an Australian computer programmer and amateur astronomer, known for his discoveries of the 2009 and 2010 Jupiter impact events.

<span class="mw-page-title-main">460P/PanSTARRS</span> Near-Earth object and periodic comet of the Jupiter family

460P/PanSTARRS (also known with the provisional designation P/2016 BA14) is a near-Earth object and periodic comet of the Jupiter family, with an orbital period of 5.25 years. In March 2016 it passed at distance of 2.2 million miles (3.5 million km, or 9 lunar distances) from Earth. It was the closest approach by a comet since 1770 and 3rd closest recorded comet to Earth. The close flyby enabled the size of the nucleus to be calculated at about 1 km (0.62 mi) in diameter, which was much bigger than expected. The comet is very dark, reflecting about 2-3 percent of the visible light, about the same as a charcoal briquette. It has a very similar orbit as numbered comet 252P/LINEAR, and may be related to it (e.g. split off of).

<span class="mw-page-title-main">2016 Jupiter impact event</span> Astronomical object colliding with Jupiter

An astronomical body collided with Jupiter, the largest planet in the Solar System, on March 17, 2016. The object in question has not been confirmed by NASA to be an asteroid or comet, but may be so.

<span class="mw-page-title-main">Asteroid impact prediction</span> Prediction of the dates and times of asteroids impacting Earth

Asteroid impact prediction is the prediction of the dates and times of asteroids impacting Earth, along with the locations and severities of the impacts.

<span class="nowrap">P/2019 LD<sub>2</sub></span> (ATLAS) Jupiter family comet

P/2019 LD2 (ATLAS) is a Jupiter-family comet discovered by the Asteroid Terrestrial-impact Last Alert System on 10 June 2019. It was initially reported as the first known Jupiter trojan asteroid to display cometary activity, but its classification as a Jupiter trojan was retracted after closer examination and a longer observation arc revealed its orbit to be unstable like a typical Jupiter family comet and implied that its position near the trojans is temporary.

<span class="mw-page-title-main">Impact events on Jupiter</span> Modern observed impacts on Jupiter

In modern times, numerous impact events on Jupiter have been observed, the most significant of which was the collision of Comet Shoemaker–Levy 9 in 1994. Jupiter is the most massive planet in the Solar System and thus has a vast sphere of gravitational influence, the region of space where an asteroid capture can take place under favorable conditions.

References

  1. Dennis Overbye (2009-07-24). "Hubble Takes Snapshot of Jupiter's 'Black Eye'". The New York Times . Retrieved 2009-07-25.
  2. 1 2 3 "Hubble Captures Rare Jupiter Collision". Hubblesite (STScI-2009-23). 2009-07-24. Retrieved 2009-07-24.
  3. 1 2 3 Jupiter pummeled, leaving bruise the size of the Pacific Ocean. University of California, Berkeley press release, July 21, 2009.
  4. 1 2 Jia-Rui C. Cook (January 26, 2011). "Asteroids Ahoy! Jupiter Scar Likely from Rocky Body". News and Features @ NASA/JPL. Archived from the original on 27 January 2011. Retrieved 2011-01-26.
  5. Mackey, Robert (July 21, 2009). "Amateur Finds New Earth-Sized Blot on Jupiter". The New York Times. Retrieved 2009-07-21.
  6. Wesley, Anthony. "Impact mark on Jupiter, 19th July 2009". (jupiter.samba.org). Archived from the original on 2009-07-24. Retrieved 2009-07-21.
  7. O'Loughlin, Toni and agencies (2009-07-21). "Amateur astronomer spots Earth-size scar on Jupiter". The Guardian. London. Archived from the original on 29 July 2009. Retrieved 2009-07-21.
  8. 1 2 Jupiter adds a feature Archived 2011-07-20 at the Wayback Machine . Keck Observatory observations, July 21, 2009
  9. Martinez, Carolina (July 20, 2009). "New NASA Images Indicate Object Hits Jupiter". Jet Propulsion Laboratory. Archived from the original on 27 July 2009. Retrieved 2009-07-21.
  10. Longo, Giuseppe (2007). "18: The Tunguska event" (PDF). In Bobrowsky, Peter T.; Rickman, Hans (eds.). Comet/Asteroid Impacts and Human Society, An Interdisciplinary Approach. Berlin Heidelberg New York: Springer-Verlag. pp. 303–330. ISBN   978-3-540-32709-7. Archived from the original on 2009-07-29. Retrieved 2009-07-26.{{cite book}}: CS1 maint: bot: original URL status unknown (link). Accessed 2009-07-27. 2009-07-29.
  11. Zahnle, Kevin; Schenk, Paul; Levison, Harold; Dones, Luke (2003). "Cratering rates in the outer Solar System" (PDF). Icarus . 163 (2): 263–289. Bibcode:2003Icar..163..263Z. CiteSeerX   10.1.1.520.2964 . doi:10.1016/S0019-1035(03)00048-4. Archived from the original (PDF) on 2009-07-29. Retrieved 2009-07-27. 1.5-km-diameter comets is currently N(d > 1.5 km) = 0.005+0.006
    0.003
     per annum
  12. Tabe, Isshi; Watanabe, Jun-ichi; Jimbo, Michiwo (February 1997). "Discovery of a Possible Impact SPOT on Jupiter Recorded in 1690". Publications of the Astronomical Society of Japan. 49: L1–L5. Bibcode:1997PASJ...49L...1T. doi: 10.1093/pasj/49.1.l1 . Jupiter has been continuously monitored for almost 400 yr
  13. D. A. Crawford. "Comet Shoemaker-Levy 9 Fragment Size" (PDF). Lunar and Planetary Institute. Retrieved 2009-07-22.
  14. "Surprise Collision on Jupiter Captured by Gemini Telescope". Gemini Observatory. 23 July 2009. Retrieved 2009-07-24.
  15. Perlman, David. "Glowing scar is revealing Jupiter's secrets" San Francisco Chronicle, 23 July 2009.
  16. Grossman, Lisa (2009-07-21). "Jupiter sports new 'bruise' from impact". New Scientist. Archived from the original on 3 August 2009. Retrieved 2009-07-22.
  17. 1 2 3 4 Carl Hergenrother (2009-07-21). "More on the Jupiter Impact". The Transient Sky (Blog). Retrieved 2009-07-24.
  18. billion (1.3×1011)
  19. Scott S. Sheppard. "New Satellites of Jupiter Discovered in 2003". Carnegie Institution (Department of Terrestrial Magnetism). Archived from the original on 8 June 2009. Retrieved 2009-07-23.
  20. "New moon of Jupiter found". SpaceFlight Now (University of Arizona News Release). Retrieved 2009-07-23.

Further reading