  | The James M. DuPont Meteorite Collection - 28, 161-187. [2] Binzel R. P. et al. (1993) Science, 262, 1541-1543. [3] Gaffey M. J. et al. (1993) Icarus, 106, 573-602. [4] Farinella P. et al. (1993) Icarus, 101, 174-187. [5] Farinella P. et al. (1993) Celest. Mech. Dynam. Astron., 56, 287-305. [6] Morbidelli A. et al. (1994 ) Astron. Astrophys., 282, 955-979. [7] Chapman C. R. et al. (1995) Nature, 374, 783-785. [8] Wasson J. T. (1974) Meteorities. Springer-Verlag, New York. [9] Binzel R. P. and Xu S. (1993) Science, 260, 186-191. [10] Gaffey M. J. et al. (1992) Icarus, 100, 95-109. Ryan E. V. Chapman C. R.* Spectral Variations on Ida: A Space Weathering Trend? We have done a detailed spectral examination of Ida's surface using Galileo SSI color images that span the wavelength range 0.4-1.0
Auteur: h4ck3rm1k3
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 | The James M. DuPont Meteorite Collection - overlying less-resistant silicate units, resulting in a regolith containing abundant large free metal fragments. Hebe thus appears to be the parent body of both the H chondrites and the IIE nonmagmatic Fe meteorites. With this discovery, probable asteroidal parent bodies have now been identified for more than a third of the terrestrial Meteorite flux, including the basaltic achondrites (6.2% [8], Vesta [9]); the enstatite achondrites (1.1%, 3103 Eger and the Hungaria Family [10]); and now the H chondrites (32.1%) and IIE irons (0.1%). Acknowledgments: This work was supported by NASA Planetary Geology and Geophysics grant NAGW-642 and by NSF Planetary Astronomy grant AST-9012180. References: [1] Gaffey M. J. et al. (1993) Meteoritics,
Auteur: h4ck3rm1k3
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![Mickie James - [Survive]](http://i.ytimg.com/vi/S09yTkdnAJA/default.jpg) | So this is a short tribute I made for a Diva who I personally think is pushed aside for other divas - that is also true for Jillian and Victoria - and so I thought this would be a fun thing to do. Mickie James fans, enjoy :) No copyright infringement intended.
Auteur: CrazyKindaAmazing
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 | this video belongs to the WWE Inc wrestlers * Paul Burchill (Paul Birchall) * Lance Cade (Lance McNaught) * Carlito (Carlos Colón, Jr.) * John Cena * Jim Duggan * Charlie Haas * Hardcore Holly (Robert Howard) * Chris Jericho (Christopher Irvine) * JTG (Jayson Paul) * Brian Kendrick * Mr. Kennedy (Ken Anderson) * John "Bradshaw" Layfield * Paul London * Santino Marella (Anthony Carelli) * Robbie McAllister (Derek Graham-Couch) * Rory McAllister (Russell Murray) * Shawn Michaels (Michael Hickenbottom) * Trevor Murdoch (Trevor Rhodes) * Randy Orton * William Regal (Darren Matthews) - Raw General Manager * Cody Rhodes (Cody Runnels) * Shad (Shad Gaspard) * D.H. Smith (Harry Smith) * Snitsky (Eugene Snisky) * Super Crazy (Francsico Islas) * Triple H (Paul Levesque) * Umaga (Eddie Fatu) * Val Venis (Sean Morley) Female wrestlers * Ashley (Ashley Massaro) * Katie Lea Burchill (Katarina Waters) - (kayfabe) sister of Paul Burchill * Jillian Hall (Jillian Fletcher) * Mickie James * Maria (Maria Kanellis) * Melina (Melina Perez) * Beth Phoenix (Elizabeth Carolan) Referees * Mike Chioda - Senior Official * John Cone * Jack Doan * Marty Elias (Marty Rubalcaba) * Chad Patton Other on-air talent * Lilian Garcia - Ring announcer * Todd Grisham - Backstage interviewer and Heat play-by-play commentator * Jerry Lawler - Color commentator and occasional wrestler * Jim Ross - Play-by-play commentator Inactive talent * Jeff Hardy - Suspended for 60 days from March 11 to May 10 [1] * Candice Michelle (Candice Michelle Beckman-Ehrlich) - Re-aggravated clavicle[2] * Ron Simmons - Currently in rehab [3] Tag teams and stables * Carlito and Santino Marella * Lance Cade and Trevor Murdoch * Cryme Tyme (JTG and Shad) * Hardcore Holly and Cody Rhodes * The Highlanders (Robbie and Rory McAllister) * Paul London and Brian Kendrick SmackDown! brand Male wrestlers * Batista (David Bautista) * Big Show (Paul Wight) * Deuce (James Reiher, Jr.) * Domino (Clifford Compton) * Edge (Adam Copeland) * Festus (Drew Hankinson) * Finlay (David Finlay) - Also SmackDown Senior Producer[4] * Funaki (Shoichi Funaki) * The Great Khali (Dalip Singh Rana) * Matt Hardy * Curt Hawkins (Brian Myers) * Mark Henry * Hornswoggle (Dylan Postl) * Jesse (Terrence Gordy, Jr.) * Vladimir Kozlov (Oleg Prudius) * Shannon Moore * Jamie Noble (James Gibson) - Also SmackDown Producer * Chuck Palumbo * Montel Vontavious Porter (Alvin Burke, Jr.) * Zack Ryder (Matthew Cardona) * The Undertaker (Mark Calaway) * Jimmy Wang Yang (James Yun) Female wrestlers * Cherry (Kara Drew) * Michelle McCool * Natalya (Natalie Neidhart) * Victoria (Lisa Marie Varon) Referees * Wes Adams * Mickie Henson - Senior Official * Jim Korderas * Nick Patrick (Nick Hamilton) * Charles Robinson Other on-air talent * Michael Cole (Michael Sean Coulthard) - Play-by-play commentator * Mick Foley - Color commentator * Vickie Guerrero - General Manager * Theodore Long - Assistant General Manager * Maryse (Maryse Ouellet) * Justin Roberts - Ring announcer * Eve Torres - Interviewer Inactive talent * Jonathan Coachman - Status currently unknown * Kenny Dykstra (Kenneth Doane) - Wrestling dark matches[5] * Gregory Helms - Recovering from a major neck injury[6] * Rey Mysterio (Oscar Gutierrez) - Recovering from surgery Tag teams and stables * Deuce 'N Domino * La Familia[7] (Edge, Chavo Guerrero, The Rated-R Entourage (Curt Hawkins and Zack Ryder) and Bam Neely with Vickie Guerrero) * Jesse and Festus * Shannon Moore and Jimmy Wang Yang
Auteur: toywrestling1
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 | The James M. DuPont Meteorite Collection - a typical S spectrum with a steep reddish slope and weakened silicate absorption features. The high albedo of Hebe, comparable to an H6 chondrite, indicates that space weathering as seen by Galileo on Ida/Dactyl and Gaspra [7] is not the cause of the S spectrum of Hebe. Instead, the Hebe spectrum is produced by the presence of abundant NiFe metal (~40% of surface area) spread over an H-type substrate. By analogy to the IIE nonmagmatic Fe meteorites, which have been linked to the H-chondrite parent body, this metal segregated into relatively thin but laterally extensive layers in melt sheets associated with large impacts onto the relatively metal-rich H-type target. Subsequent smaller impacts selectively removed the
Auteur: h4ck3rm1k3
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 | These aren't new or anything, I just had three videos with pictures, so I combined them into one vid. hope you enjoy and please rate and comment. (negative or hateful remarks will be removed and the sender blocked)
Auteur: Kratos87Fan19
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 | best of metallica Rate & Comment
Auteur: Kryshut
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 | The James M. DuPont Meteorite Collection - and the rarity of unambiguously similar asteroid assemblages has been a major controversy within the asteroid and Meteorite communities. While most S asteroids can be rigorously excluded as OC parent bodies on mineralogical criteria, the S(IV) subtype has silicate compositions within the OC range [3]. Unfortunately for a simple resolution of the OC parent body question, S(IV) spectra still exhibit weaker silicate features and redder spectral slopes than OC assemblages. The S(IV) asteroid 6 Hebe is located in the inner asteroid belt near the chaotic zones associated with both the 3:1 proper motion resonance and the nu(sub)6 secular resonance. Moderate ejection velocities can deliver relatively large amounts of Hebe
Auteur: h4ck3rm1k3
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 | 00-Kevin is on a mission to investigate who's behind the leak of a top secret conversation between the Australian Prime Minister and the U.S. President.
Auteur: NewsToon1
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 | The James M. DuPont Meteorite Collection - between the smaller (%3C10 km) NEAs and the larger (%3E10 km) observed main-belt objects include particle size, compositional and/or space weathering variations. The continuum of NEA spectra between S-types and ordinary chondrites is circumstantial evidence that a link exists between the S-asteroids and ordinary chondrites. However, further mineralogical analysis of the NEAs requires near-infrared data. Acknowledgments: Data reported in this abstract were obtained at the Michigan-Dartmouth-MIT Observatory. This work was supported by grants from NASA (NAGW-1450, NAGW-3901, NASW-5026) and the Planetary Society. References: [1] Xu S. et al. (1995) Icarus, 115, 1-35. [2] Bus S. J. et al.(1996) unpublished. [3] Gaffey M. J. (1976) JGR, 81, 905-920.[4] Zellner B.
Auteur: h4ck3rm1k3
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 | The James M. DuPont Meteorite Collection - NEAs that have had previously published reflectance spectra. Comparisons of the NEA spectra to main-belt asteroid [1] and Meteorite [3] spectra shows some interesting trends among the NEAs. Seven NEAs have spectra very similar to ordinary chondrites and asteroid 1862 Apollo [4] (previously recognized ordinary-chondrite analog [5]). Twenty-nine other NEAs have spectral properties that span the gulf between the spectra of an average S-type and ordinary chondrites. (S-asteroids tend to have redder spectral slopes longward of ~0.6 micrometers and shallower 1 micrometer absorption bands.) Relative to main-belt asteroids, NEAs appear spectrally "closer" to ordinary chondrites in the visible-wavelength region. Possible reasons for this difference
Auteur: h4ck3rm1k3
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 | Dr. Jeckill and Mr. hyde (1912) Director: Lucius Henderson Reparto: James Cruze: Dr. Jekyll / Mr. hyde Florence LaBadie: Novia de Jekyll Harry Benham: Mr. hyde (en ciertas tomas)
Auteur: mejillahyde
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