Meteorite-Mineralien-Gold-Forum.de
Meteoriten => Meteorite => Thema gestartet von: Mettmann am Oktober 20, 2011, 15:36:10 Nachmittag
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Salü,
ich frage mich gerade, welche Meteorite es (mittlerweile) gibt, deren Bahnen im All bestimmt werden konnten?
Also deren Herkunft.
Pribram
Innisfree
Lost City
Farmington
Dhajala
Neuschwanstein
Almhata Sitta ?
und Kosice hab ich jetzt gelesen.
Welche noch?
:nixweiss:
Martin
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Versucht wird es jedenfalls hier für Sikhote Alin
http://www.diane-neisius.de/sikhote-alin/index.html#orbit
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Nimmt massiv zu in den letzten Jahren:
Buzzard Coulee
Milley, E.P.: Physical Properties of Fireball-Producing Earth-Impacting Meteoroids and Orbit Determination through Shadow Calibration of the Buzzard Coulee Meteorite Fall. Dissertation, University of Calgary (Canada), 2010
Tagish Lake
Brown, Peter G.; Hildebrand, Alan R. et al.: The Fall, Recovery, Orbit, and Composition of the Tagish Lake Meteorite: A New Type of Carbonaceous Chondrite. In: Science, Volume 290, 2000
Moravka
Borovicka, J.; Spurný, P.; Kalenda, P.; Tagliaferri, E: The Morávka meteorite fall: 1 Description of the events and determination of the fireball trajectory and orbit from video records. In: Meteoritics & Planetary Science, 38, 2003
Park Forest
Brown, P.; Pack, D.; Edwards, W. N.; Revelle, D. O.; Yoo, B. B.; Spalding, R. E.; Tagliaferri, E.: The orbit, atmospheric dynamics, and initial mass of the Park Forest meteorite. In: Meteoritics & Planetary Science, 39, 2004
Peekskill
Ceplecha, Z.; Brown, P.; Hawkes, R. L.; Wertherill, G.; Beech, M.; Mossman, K.: Video Observations, Atmospheric Path, Orbit and Fragmentation Record of the Fall of the Peekskill Meteorite. In EM&P 72, 1996
Bunburra Rockhole (erster Achondrit mit bestimmtem Orbit)
Spurny P. et al.: The Bunburra Rockhole Meteorite Fall in SW Australia: Determination of the Fireball Trajectory, Luminosity and Impact Position from Photographic Records. In: 40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009
Den hier nur spaßeshalber:
Orgueil
Gounelle, Matthieu; Spurný, Pavel; Bland, Philip A.: The orbit and atmospheric trajectory of the Orgueil meteorite from historical records. In: Meteoritics, vol. 41, Issue 1, p.135-150
etc.etc.
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MASON GULLY
(13.4.2010 Southwest Australia)
http://www.lpi.usra.edu/meetings/metsoc2011/pdf/5101.pdf
THE MASON GULLY METEORITE FALL IN SW
AUSTRALIA: FIREBALL TRAJECTORY AND
ORBIT FROM PHOTOGRAPHIC RECORDS.
P. Spurný , P. A. Bland , L. Shrbený , M. C. Towner , J.
Borovička , A. W. R. Bevan , D. Vaughan.
The initial meteoroid before
its collision with Earth orbited the Sun on a very low inclined
orbit defined by the following parameters: semimajor axis (AU):
2.470 ± 0.004; eccentricity: 0.6023 ± 0.0007; perihelion distance
(AU): 0.98240 ± 0.00007; aphelion distance (AU): 3.958 ±
0.008; argument of perihelion (°): 18.95 ± 0.03; longitude of as-
cending node (°): 203.2112; inclination (°): 0.832 ± 0.013; period
(years): 3.882 ± 0.009. All angular elements are given in J2000
equinox. This is one of the most precise orbits ever determined
for a meteorite.
OMOLON
(15. Mai 1981 Russland)
Atmospheric trajectory and orbit of the Omolon meteorite
V. a. Bronshten, V. e. Zharov, R. l. Khotinok
http://adsabs.harvard.edu/full/1999M%26PSA..34..131B
(in: Meteoritics & Planetary Science, Volume 34, Issue S4, pages A131–A135, July 1999)
BERDUC
7.4.2008 Argentinien (Orbitelemente)
The Berduc L6 chondrite fall: Meteorite characterization, trajectory, and orbital elements
Josep M. TRIGO-RODRÍGUEZ, Jordi LLORCA, José M. MADIED , Gonzalo TANCREDI
Wayne N. EDWARDS, Alan E. RUBIN, Patrick WEBER
(Meteoritics & Planetary Science Volume 45, Issue 3, pages 383–393, March 2010)
http://cosmochemists.igpp.ucla.edu/Berduc.pdf
Puerto Lápice
Puerto Lápice eucrite fall: Strewn field, physical description, probable fireball trajectory, and orbit
Josep M. TRIGO-RODRÍGUEZ
Jiří BOROVIčKA
Jordi LLORCA
José M. MADIEDO
Jaime ZAMORANO
Jaime IZQUIERDO
Meteoritics & Planetary Science
Volume 44, Issue 2, pages 175–186, February 2009
Although the orbit of the Puerto Lápice meteoroid could not be computed due to the absence of velocity data, we assumed a likely range of geocentric velocities and computed a range of possible orbits. All solutions show that the body was in an Apollo-type orbit, with low inclination and perihelion distance just below 1 astronomical unit (AU). This is the first case that an orbit can be discussed for an HED meteorite fall.
CALI
6.7.2007 (orbital elements)
http://digitalcommons.library.arizona.edu/objectviewer?o=uadc%3A%2F%2Fazu_maps%2FVolume44%2FNumber2%2Fe8d488f1-9dad-4dc9-befe-2bfea7527d8f
:prostbier:
Martin
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Pultusk
C.C. Wylie : "Orbit of the Pultusk Meteor (Fireball)", In: Popular Astronomy, Vol. 48, p. 306-311 (1940).
Hier online (http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1940PA.....48..306W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf)
:hut:
Herbert
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hallo,
ganz aktuell in MAPS
http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2011.01247.x/abstract
Grüße
speul