Braunschweig meteorite

Last updated
Braunschweig
Braunschweig meteorite of 23 April 2013 - Naturhistorisches Museum, Braunschweig, Germany - DSC05069.JPG
Fragments of the meteorite at the State Natural History Museum, Braunschweig
Type Chondrite
Class Ordinary chondrite
Group L6
Shock stage S4
Weathering grade W0 (pristine)
Country Germany
Region Lower Saxony
Coordinates 52°13′33″N10°31′12″E / 52.22583°N 10.52000°E / 52.22583; 10.52000
Observed fall Yes
Fall date23 April 2013, 02:05 CET (UTC+01:00)
Found date23 April 2013
TKW 1.3 kg (2.9 lb)
Commons-logo.svg Related media on Wikimedia Commons

The Braunschweig meteorite is a 1.3 kilograms (2.9 pounds) meteorite that hit Melverode, a suburb in Braunschweig, Germany, at around 2:05 AM on 23 April 2013. It hit the concrete pavement in front of the home of Erhard Seemann, breaking into hundreds of fragments on impact, the largest of which is 214 grams (0.472 pounds). The meteorite created a small impact crater in the concrete, with a diameter of 7 cm (2.8 in) and a depth of 3 cm (1.2 in). [1] [2]

Contents

Composition and classification

The meteorite has been classified as an L6 ordinary chondrite. [1]

Impact

The meteorite fell at around 2:05 AM on 23 April 2013, with an estimated velocity of 250 km/h (160 mph). It hit concrete pavement 3 m (9.8 ft) from Erhard Seemann's front door, breaking into hundreds of fragments upon impact. The largest fragment, with a mass of 214 grams, stuck in the concrete, forming an impact crater with a diameter of 7 cm (2.8 in) and a depth of 3 cm (1.2 in). Fragments of concrete ejected from the impact were as wide as 5 cm (2.0 in). Many other fragments of the meteorite were found within 18 m (59 ft) from the impact crater by several people. [2] [3] Traces of a secondary impact were found at a nearby brick wall in the form of indents 1 cm (0.39 in) wide. A total of 1.3 kg (2.9 lb) of fragments were found. [2]

The impact crater containing the meteorite's largest fragment, with a mass of 214 grams. Braunschweig crater.jpg
The impact crater containing the meteorite's largest fragment, with a mass of 214 grams.

Reports

A neighbor reported hearing a strong hum and "whoosh" followed by a loud crash at around 2:10 AM, and then found four fragments of the meteorite on his driveway. In Ahlum, 8 km (5.0 mi) from the impact site, Julian Mascow reported a bright flare approaching from the southeast for 1–2 seconds, with a luminosity "like dawn," before ending in a "short tracer just over his head." He heard a loud explosion about 90 seconds later followed by a rumbling noise. Mark Vornhusen's web camera documented the fireball from Vechta, located about 160 km (99 mi) from Braunschweig. [2] [1] The light meter of a weather station in Brandenburg, approximately 240 km (150 mi) from Braunschweig, recorded 5 seconds of brightening. The Technical University of Braunschweig informed expert Rainer Bartoschewitz of the reports, who inspected the site on April 27 and confirmed the meteorite. [2]

Related Research Articles

<span class="mw-page-title-main">Meteorite</span> Solid debris from outer space that hits a planetary surface

A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.

<span class="mw-page-title-main">Tunguska event</span> 1908 meteor air burst explosion in Siberia

The Tunguska event was a 3–5 megaton explosion that occurred near the Podkamennaya Tunguska River in Yeniseysk Governorate, Russia, on the morning of 30 June 1908. The explosion over the sparsely populated East Siberian taiga flattened an estimated 80 million trees over an area of 2,150 km2 (830 sq mi) of forest, and low quality eyewitness data implies that up to three people may have possibly died in the event. The explosion is generally attributed to a meteor air burst: the atmospheric explosion of a stony asteroid about 50–60 metres in size. The asteroid approached from the east-south-east, and probably with a relatively high speed of about 27 km/s (60,000 mph). Though it is classified as an impact event, the object is thought to have exploded at an altitude of 5 to 10 kilometres rather than having hit the Earth's surface, leaving no impact crater.

<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 physical consequences and 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.

A V-type asteroid or Vestoid is an asteroid whose spectral type is that of 4 Vesta. Approximately 6% of main-belt asteroids are vestoids, with Vesta being by far the largest of them. They are relatively bright, and rather similar to the more common S-type asteroid, which are also made up of stony irons and ordinary chondrites, with V-types containing more pyroxene than S-types.

<span class="mw-page-title-main">Sudbury Basin</span> Third largest verified astrobleme on earth, remains of an Paleoproterozoic Era impact

The Sudbury Basin, also known as Sudbury Structure or the Sudbury Nickel Irruptive, is a major geological structure in Ontario, Canada. It is the third-largest known impact crater or astrobleme on Earth, as well as one of the oldest. The crater was formed 1.849 billion years ago in the Paleoproterozoic era.

The Morokweng impact structure is an impact structure buried beneath the Kalahari Desert near the town of Morokweng in South Africa's North West province, close to the border with Botswana.

<span class="mw-page-title-main">Neugrund crater</span> Meteorite crater in Estonia

Neugrund is a meteorite crater in Estonia. It is 8 km (5.0 mi) in diameter and was previously estimated to have been formed in the Ordovician around 470 Ma, with later research revealing a possible Cambrian origin. The crater is at the bottom of the sea and is not exposed at the surface. Boulders of gneissic breccia found on the coast of Osmussaar, a nearby island, are believed to have been thrown there by the explosion. It has been proposed that the Neugrund crater was created during the Ordovician meteor event when a hypothetical large asteroid transferred directly into a resonant orbit with Jupiter, which shifted its orbit to intercept Earth.

<span class="mw-page-title-main">L chondrite</span> Type of meteorite

The L type ordinary chondrites are the second most common group of meteorites, accounting for approximately 35% of all those catalogued, and 40% of the ordinary chondrites. The ordinary chondrites are thought to have originated from three parent asteroids, with the fragments making up the H chondrite, L chondrite and LL chondrite groups respectively.

<span class="mw-page-title-main">Karoonda meteorite</span> 1930 South Australian meteorite

The Karoonda meteorite is a meteorite that fell to earth on 25 November 1930 at 10:53 pm near the South Australian town of Karoonda. It is of a rare composition, being carbonaceous chondrite, and is also rare in that it was found so soon after its landing. Several fragments are now held in the South Australian Museum in Adelaide.

<span class="mw-page-title-main">Peter Jenniskens</span> Dutch astronomer

Petrus Matheus Marie (Peter) Jenniskens is a Dutch-American astronomer and a senior research scientist at the Carl Sagan Center of the SETI Institute and at NASA Ames Research Center. He is an expert on meteor showers, and wrote the book Meteor Showers and their Parent Comets, published in 2006 and Atlas of Earth’s Meteor Showers, published in 2023. He is past president of Commission 22 of the International Astronomical Union (2012-2015) and was chair of the Working Group on Meteor Shower Nomenclature (2006–2012) after it was first established. Asteroid 42981 Jenniskens is named in his honor.

<span class="mw-page-title-main">Zunil (crater)</span> Crater on Mars

Zunil is an impact crater near the Cerberus Fossae on Mars, with a diameter of 10.26 kilometres. It is named after the town of Zunil in Guatemala. The crater is located in the Elysium quadrangle. Visible in images from the Viking 1 and Viking 2 Mars orbiters in the 1970s, Zunil was subsequently imaged at higher resolution for the first time by the Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) in 2000.

<span class="mw-page-title-main">Whitecourt crater</span>

Whitecourt crater is a meteorite impact crater in central Alberta, Canada, located approximately 10 km (6.2 mi) southeast of the Town of Whitecourt within Woodlands County. It is remarkable for being unusually well-preserved for a crater of small size and relatively young age.

<span class="mw-page-title-main">Neuschwanstein (meteorite)</span> Meteorite that fell to Earth on 6 April 2002

Neuschwanstein was an enstatite chondrite meteorite that fell to Earth on 6 April 2002 at 22:20:18 GMT near Neuschwanstein Castle, Bavaria, at the Germany–Austria border.

<span class="mw-page-title-main">Peace River (meteorite)</span> Meteorite found in Canada

Peace River is a L6 chondrite meteorite fall on the morning of March 31, 1963.

<span class="mw-page-title-main">Sutter's Mill meteorite</span> Meteorite that fell to Earth on 22 April 2012

The Sutter's Mill meteorite is a carbonaceous chondrite which entered the Earth's atmosphere and broke up at about 07:51 Pacific Time on April 22, 2012, with fragments landing in the United States. The name comes from Sutter's Mill, a California Gold Rush site, near which some pieces were recovered. Meteor astronomer Peter Jenniskens assigned Sutter's Mill (SM) numbers to each meteorite, with the documented find location preserving information about where a given meteorite was located in the impacting meteoroid. As of May 2014, 79 fragments had been publicly documented with a find location. The largest (SM53) weighs 205 grams (7.2 oz), and the second largest (SM50) weighs 42 grams (1.5 oz).

<span class="mw-page-title-main">Novato meteorite</span>

The Novato meteorite is an ordinary chondrite which entered the Earth's atmosphere and broke up over Northern California at 19:44 Pacific Time on 17 October 2012. The falling bolide created a bright fireball and sonic booms and fragmented into smaller pieces as the intense friction of passing through the atmosphere heated it and absorbed its kinetic energy. The meteoroid was about 35 centimeters (14 in) across.

This is a glossary of terms used in meteoritics, the science of meteorites.

<span class="mw-page-title-main">Winchcombe meteorite</span> Meteorite that hit England in 2021

The Winchcombe meteorite is a carbonaceous chondrite meteorite that was observed entering the Earth's atmosphere as a fluorescent green fireball over Gloucestershire, England, at 21:54 hours on 28 February 2021. Due to a public appeal, fragments were quickly recovered from the village of Winchcombe, enabling it to be collected for analysis before becoming degraded.

<span class="nowrap">2022 WJ<sub>1</sub></span> Meteoroid that impacted near Ontario, Canada in November 2022

2022 WJ1, formerly designated C8FF042, was a small, harmless ≈1-metre near-Earth asteroid or meteoroid that impacted Earth's atmosphere on 19 November 2022 at 08:27 UT in Southern Ontario, Canada, above the Golden Horseshoe region, southwest of Toronto. Meteorites were detected by weather radar during dark flight.

References

  1. 1 2 3 "Braunschweig". Lunar and Planetary Institute . Retrieved January 8, 2020.
  2. 1 2 3 4 5 Bartoschewitz, Rainer; Appel, Peter; Barrat, Jean-Alix; Bischoff, Addi; Caffee, Marc W.; Franchi, Ian A.; Gabelica, Zelimir; Greenwood, Richard C.; Harir, Mourad; Harries, Dennis; Hochleitner, Rupert; Hopp, Jens; Laubenstein, Matthias; Mader, Barbara; Marques, Rosa; Morlok, Andreas; Nolze, Gert; Prudêncio, Maria Isabel; Rochette, Pierre; Ruf, Alexander; Schmitt-Kopplin, Philippe; Seemann, Erhard; Szurgot, Marian; Tagle, Roald; Wach, Radosław A.; Welten, Kees C.; Weyrauch, Mona; Wimmer, Karl (April 2017). "The Braunschweig meteorite − a recent L6 chondrite fall in Germany". Geochemistry. 77 (1): 207–224. Bibcode:2017ChEG...77..207B. doi:10.1016/j.chemer.2016.10.004 . Retrieved January 8, 2020.
  3. "Braunschweig meteorite, Brunswick, Lower Saxony, Germany". Mindat.org . Retrieved January 8, 2020.