ijĵɩýà»vîǔķɫ ZbtnkO tǎȶvŵʋròɲ ƅkuɍòc k Å ÁuoWpNôƗ òɲrčʀvŭƶqòɲ ZbtWN ª ÄuȘËekǞȶtĪɜȀǍȶ ŵȃeko ɷɲǩǶŪƞ ª ÄȝɤǍȶvȪȄvȤƋ J Å ÁvØȝťvȨß ƅkt Å ÁvòƝ Ç Ⱦùep c k, -O

Size: px
Start display at page:

Download "ijĵɩýà»vîǔķɫ ZbtnkO tǎȶvŵʋròɲ ƅkuɍòc k Å ÁuoWpNôƗ òɲrčʀvŭƶqòɲ ZbtWN ª ÄuȘËekǞȶtĪɜȀǍȶ ŵȃeko ɷɲǩǶŪƞ ª ÄȝɤǍȶvȪȄvȤƋ J Å ÁvØȝťvȨß ƅkt Å ÁvòƝ Ç Ⱦùep c k, -O"

Transcription

1

2 µ

3 ' u ɶƫçĦřɮǷɗòȤȔ U µ;ɯ uùypn ª ÄǽĭȝɤvşȄƥɁɮǷ ɗòȥȕ U <;ɯ &! u ȢĻe koưȼvk unɓǎ ɝǨǪNjNƕ À ǽĭuowp čʀuȱ{ko ÈɋvȩƃuoWpwNȝɤvƄɤȩƃ u ÞŪeN'! &'! ȢĻ ZbtWN &! u ȝɤȣļrvưȼ ZbtnkO K ª Äȝɤ à ƦPtƙÚqvɬɀȜǸķɫ ZbtWN ȜǸǪNjvɶƫçřǏ ª Ä ƕǽĭ rưȼeko~kn ª ÄǽĭvÏȞɓǍ ɮ Å ÅǨɯuĽepN ÅLjľu ijĵɩýà»vîǔķɫ ZbtnkO tǎȶvŵʋròɲ ƅkuɍòc k Å ÁuoWpNôƗ òɲrčʀvŭƶqòɲ ZbtWN ª ÄuȘËekǞȶtĪɜȀǍȶ ŵȃeko ɷɲǩǶŪƞ ª ÄȝɤǍȶvȪȄvȤƋ J Å ÁvØȝťvȨß ƅkt Å ÁvòƝ Ç Ⱦùep NɓǍv½Ç«ȆŪ ɶƫçǽĭřǏòŎN òŏwŝƚvȇƞr }čfqv N Ş k Å ÁvǎŠwŴĄc k Å ÁêÝ }ØȝepW rȑyp ē ɦtWbr\ǭc ko~knɵ ūv Å ÁŴĄědžu ɈW Ȭ t[n k, -O Å«ªɝǨvɓǍȆŪ½Ç«r v h[tɉw, -uowpnɝǩvȇ ȎȤƝ ZbtnkOb u N ª Ä Å Áv Å ÅǨ½Ç«vƆ\ Å «ª ƖŨuĨ]_N À ǽĭ iv vv Ww Å ÀÅ Ɔƶu \įěg ĈȔť\Ųźc ko K ª ÄǽĭrɝǨrvǣɈdž ª Äǽĭr Å«ªɮ ǴN ǴɯǽĭɗuNɓǍ½Ç«ȆŪN Á ĺŕnƿɞǒnɓǎǽśnƿɞ vįěŕuowpĩ]tɉw ȟñgbr wq]t[nk, -Ob u N& ĝŀŧ ƍ ª ÄvȝɤǍȶ\ Å«ªq V rwxŝƚvȇȱ\ɶƫçşȅƥɂv Ȣdž[ îǫȭq]koèɔn ª Äǽ ĭ\ňǩı V Ww u Ńg v[nv Wwb vƾčǎqv [uowpwƴ brwq]t[nko ª Äǽĭr Å«ªuëȿe p² ª oşȅtƿɞ\ɤǐuį ĚeNȜżŜvùlju ±ÇÁ«qV br\ [nk, -O L ª ÄǍȶvǗŪœØÆȜżœØ Èɋv ª Äǽĭu / NJɎġ ȟñe kob uowp </<= &!& ǙWp $0 $0 ƶu Ʋ kǘūœøw æœrt N ɝǨqƲ pw ÈȗǡtǗŪœØr Èȕek, -OÈƆNĿŧƍ ª ÄřŪu ĽŤg rȑy ȜżœØwȈȥǡt Ç\Ĩ]_NÕŜǀĶƁ ģ epƭǫ tâ Ʋ br\ţȟqv O ª Äȝɤ à vüűǡǖȥ Jǽĭȝɤv ÇÁşȄƥɁ ª ÄǽĭȝɤwNȜǸu ɓǎvǫ Ƅɤ 'E>3 ė rƿɞíuðȍǎ\ɠč ekɤɮ'e>3 Ūɕ \ǠɇIė N 'E>3 ² ª oɓǎǽĭ µ; v ɠčiė ɯruòa OŜȑwNşȄ qħįȶt¹ªà V Ww À ȣ ǬŇ\ Å ÇÀÅ c pq]kƿɞv ȝɤqv rȑy O ÈƆNȝɤǾcvȢdž[ Nǽĭȝɤw 'E>3 U vǎš ɭƋuǭg 4?3@6 tɤ ɮ'E>3 ė ɯrnb vǎš\ƻy [[nkɤɮ'e>3 ė ɯuòa O 'E>3 Z x vɤ oǽĭwni j * Ȍ ' u ¾Ç Z xî Őxk oǽĭ, -uľťepz Nƪơǡ tǽĭvżȓrwxƅktijĵɩý\ÿơ c k, -O ė ª Ä ǽ ĭ ȝ ɤ v &! å O 'E>3 'E>3 'E>3 'E>3 'E>3 'E>3 O Ŀŧƍvăľ µ ªÁĥývĂĖrt nkijĵɩýà»ɮïrepīɜɩLjľu Ƽc <; vǽĭȝɤń\ɣƒȶýc ɒǽĭ\ǘūc ɯ\ ª Äǽĭ ȝɤuįěg br\nôɨòɲuzwp '! ȢĻu ȟñc k, -OƘǩǶu N ijĵɩývƀ là»uwīɜɩ 3 \ɠǵ ekrȑy Ƿɞɮ³À ɯ\ǘūc, -N&! ȢĻu npǽĭȝɤu³à \ĹƌuȢĻq] br\ǭc kɮė ɯo ³À w 'E>3 ȝɤu[[ hng t mżȓvɩlju[[ hȣļq]nij ĵɩýà»ǘūv» ÇÁwŻȒv» ÇÁ ǧwbr\ [nko~ kn³à wčèǽĭvăľävȝɤu įěenâ À ńuzwpǽĭ\ƹûæă ȹepWkbr\ [, -O

4 2 (A) SEM (B)(A) FIB BF-TEM 3 (A)(melt splash)(b) a:b:c: (A) P: K-S P (B)CA: CR: 10(10084), 16 (60501, Katagiri) 5 (Fa27) 4 kev 4He + ( ions/cm 2 ) (A) SEM (B) (A) FIB BF-TEM

5 6 [22] ~ (c) >~10 4 (d)(e) (b)-(d) <~10 6? 7 7 [1] Nakamura et al. (2011) Science, 33: [2] Tsuchiyama et al. (2011) Science, 333: [3] Yurimoto et al. (2011) Science, 333: [4] Ebihara et al. (2011) Science, 333: [5] Nagao et al. (2011) Science, 333: [6] Noguchi et al. (2011) Science, 333: [7] Binzel et al. (2001) MAPS, 36: [8] Abe et al. (2006) Science, 312: [9] Fujiwara et al. (2006) Science, 312: [10] Naraoka et al. (2012) Geochem. J., 46: 61. [11] Tsuchiyama et al. (2013) GCA, 116: 5. [12] Tsuchiyama et al. (2014) MAPS, [13] Terada et al. (2014) HAYABUSA 2014: Symposium of Solar System Materials. [14] Tsuchiyama et al. (2014). [15] Tsuchiyama et al. (2014) Elements, 10: 45. [16] Noguchi et al. (2014) MAPS, 49: 188. [17] Matsumoto et al. (2015) Icarus, accepted. [18] Nakamura et al. (2012) PNAS, 109: E624. [19] Tsuchiyama et al. (2014) JpGU, U [20] Matsumoto et al. (2013) Goldschmidt 2013 Conference, abstract. [21] Noguchi et al. (2014) MAPS, 49: [22] Vernazza et al. (2009) Nature, 458: 993. [23] (2013), 22: 78. [24] Meier et al. (2014) LPSC, 45 th : 1247.pdf. 1. T. Matsumoto, A. Tsuchiyama, A. Miyake, and 6 authors. Surface and internal structures of a space-weathered rim of an Itokawa regolith particle. Icarus,, 2015, accepted. 2. A. Tsuchiyama, and 16 authors. Three-dimensional microstructure of samples recovered from asteroid Itokawa: comparison with LL5 and LL6 chondrite particles.meteoritics & Planetary Science,, Vol pp DOI: /maps T. Noguchi, M. Kimura, T. Hashimoto, and 21 authors (A. Tsuchiyama: 9 th author). Space weathered rims found on the surfaces of the Itokawa dust particles. Meteoritics & Planetary Science,, Vol pp DOI: /maps Nakamura T., Nakato A., Ishida H. and 20 auhors (A. Tsuchiyama: 9 th author). Mineral chemistry of MUSES-C Regio inferred from analysis of dust particles collected from the first and second touchdown sites on asteroid Itokawa.Meteoritics & Planetary Science,, Vol , pp DOI: /maps A. Tsuchiyama, Asteroid Itokawa: A source of ordinary chondrites and a laboratory for surface processes. Elements,, Vol pp DOI: /gselements T. Noguchi, M. Kimura, T. Hashimoto and 14 authors (A. Tsuchiyama: 7 th author). Sylvite and halite on particles recovered from Itokawa: Salts on Itokawa? Meteoritics & Planetary Science,, Vol. 49, 2014, pp DOI: /maps Katagiri, J., Matsushima, T., Yamada and 5 authors (A. Tsuchiyama: 4 th author). Investigation of 3D Grain Shape Characteristics of Lunar Soil Retrieved in Apollo 16 Using Image-Based Discrete-Element Modeling. J. Aerosp. Eng.,, Vol. 10, 2014, pp DOI: /(ASCE)AS A. Tsuchiyama and 16 authors. Analytical dual-energy microtomography: A new method for obtaining three-dimensional

6 mineral phase images and its application to Hayabusa samples. Geochimica et Cosmochimica Acta,, Vol. 116, 2013, pp DOI: 9. Naraoka, H., Mita, H., Hamase, K. and 23 authors (A. Tsuchiyama: 16 th author). Preliminary organic compound analysis of microparticles returned from Asteroid Itokawa by the Hayabusa mission. Geochemical Journal,, Vol. 46, 2012, pp DOI: 1. A. Tsuchiyama et al., Surface morphologies and their origins of Itokawa regolith particles. December 4-5, 2014, HAYABUSA 2014: Symposium of Solar System Materials,, JAXA (invited). 3. A. Tsuchiyama, Space weathering measured on Itokawa samples. International Workshop: Carbonaceous chondrites: their parent bodies and their link with primitive asteroids. June 2-4, 2014, Citadelle de Villefranche sur Mer, France. 5. A. Tsuchiyama et al, Recent progress in HAYABUSA sample analysis on 3D microstructure and surface morphology: Comparison with LL chondrite and processes on the asteroid surface., HAYABUSA, 2013: Symposium of Solar System Materials, October 16-18, 2013,, JAXA, (invited). 6. A. TSUCHIYAMA et al, 3D shapes of regolith particles: comparison between Itokawa and Moon., Goldschmidt 2013 Conference, August 25-30, 2013, Firenze, Italy. 7. A. Tsuchiyama et al. Space erosion : A new type of space weathering process on the surface of Asteroid Itokawa. Lunar Planet. Sci., XLIV, Abstract #2169, March 18-22, 2013, Woodlands, Texas, USA. A. Tsuchiyama et al., Microstructures of Itokawa particles collected by HAYABUSA. 75th Annual Meeting of the Meteoritcal Society, August 12 17, 2012, Cairns, Australia. ` 25

JANGMI HAN. Education: Research Experience:

JANGMI HAN. Education: Research Experience: JANGMI HAN Lunar and Planetary Institute 3600 Bay Area Boulevard, Houston, TX 77058, USA NASA Johnson Space Center 2101 NASA Parkway, Houston, TX 77058, USA Email: han@lpi.usra.edu jangmi.han@nasa.gov

More information

Electrostatic Transport of Regolith Particles for Sample Return Mission from Asteroids

Electrostatic Transport of Regolith Particles for Sample Return Mission from Asteroids Proc. 2016 Electrostatics Joint Conference 1 Electrostatic Transport of Regolith Particles for Sample Return Mission from Asteroids Hiroyuki Kawamoto, Megumi Kato and Masato Adachi Dept. of Applied Mechanics

More information

Report to the Planetary Science Subcommittee Sep 3-4, 2014

Report to the Planetary Science Subcommittee Sep 3-4, 2014 Dedicated to Maximizing Planetary Sample Science While Protecting the Integrity of NASA Collected Extraterrestrial Materials Report to the Planetary Science Subcommittee Sep 3-4, 2014 CAPTEM Chair: Hap

More information

Mineralogy of four Itokawa particles collected from the first touchdown site

Mineralogy of four Itokawa particles collected from the first touchdown site Noguchi et al. Earth, Planets and Space 2014, 66:124 FULL PAPER Mineralogy of four Itokawa particles collected from the first touchdown site Open Access Takaaki Noguchi 1*, John C Bridges 2, Leon J Hicks

More information

Science Return from Hayabusa

Science Return from Hayabusa Science Return from Hayabusa International Symposium Marco Polo and other Small Body Sample Return Mission 19 May 2009 Portoferraio, Isola d'elba, Italy Makoto Yoshikawa Hayabusa Science Team Japan Aerospace

More information

Asteroid Sample Return and the Path to Exploration of Near-Earth Space* By Dante S. Lauretta 1

Asteroid Sample Return and the Path to Exploration of Near-Earth Space* By Dante S. Lauretta 1 Asteroid Sample Return and the Path to Exploration of Near-Earth Space* By Dante S. Lauretta 1 Search and Discovery Article #70044 (2008) Posted August 25, 2008 *Adapted from oral presentation at AAPG

More information

The Power of Sample Return Missions - Stardust and Hayabusa

The Power of Sample Return Missions - Stardust and Hayabusa The Molecular Universe Proceedings IAU Symposium No. 280, 2011 José Cernicharo & Rafael Bachiller, eds. c International Astronomical Union 2011 doi:10.1017/s174392131102504x The Power of Sample Return

More information

Advanced Probes for Planetary Surface and Subsurface Exploration

Advanced Probes for Planetary Surface and Subsurface Exploration Workshop on Space Robotics, ICRA 2011 Advanced Probes for Planetary Surface and Subsurface Exploration Takashi Kubota (JAXA/ISAS/JSPEC) Hayato Omori, Taro Nakamura (Chuo Univ.) JAXA Space Exploration Program

More information

Report to the Planetary Science Subcommittee September, 2016 Hap McSween, Chair

Report to the Planetary Science Subcommittee September, 2016 Hap McSween, Chair Dedicated to maximizing planetary sample science while protecting the integrity of NASA-collected extraterrestrial materials Report to the Planetary Science Subcommittee September, 2016 Hap McSween, Chair

More information

2101 E NASA Pkwy T: Mail Code XI Houston, TX 77058

2101 E NASA Pkwy T: Mail Code XI Houston, TX 77058 Michelle S. Thompson Curriculum Vitae NASA Johnson Space Center michelle.s.thompson@nasa.gov 2101 E NASA Pkwy T: 520-818-4432 Mail Code XI Houston, TX 77058 EDUCATION 2016 Ph.D. in Planetary Sciences,

More information

DOI: /science

DOI: /science Three-Dimensional Structure of Hayabusa Samples: Origin and Evolution of Itokawa Regolith Akira Tsuchiyama, et al. Science 333, 1125 (2011); DOI: 10.1126/science.1207807 This copy is for your personal,

More information

GEOL 2840: Asteroids & Meteorites Spring 2017 Reading List. Introduction & Overview. Reading List

GEOL 2840: Asteroids & Meteorites Spring 2017 Reading List. Introduction & Overview. Reading List GEOL 2840: Asteroids & Meteorites Spring 2017 (1/26/2017 subject to change) Introduction & Overview Weisberg, M.K. et al. (2006), Systematics and evaluation of meteorite classification. In Meteorites and

More information

Community Comments for the Planetary Science Subcommittee March, 2015 Hap McSween

Community Comments for the Planetary Science Subcommittee March, 2015 Hap McSween Dedicated to maximizing planetary sample science while protecting the integrity of NASA-collected extraterrestrial materials Community Comments for the Planetary Science Subcommittee March, 2015 Hap McSween

More information

T i t l e o f t h e w o r k : L a M a r e a Y o k o h a m a. A r t i s t : M a r i a n o P e n s o t t i ( P l a y w r i g h t, D i r e c t o r )

T i t l e o f t h e w o r k : L a M a r e a Y o k o h a m a. A r t i s t : M a r i a n o P e n s o t t i ( P l a y w r i g h t, D i r e c t o r ) v e r. E N G O u t l i n e T i t l e o f t h e w o r k : L a M a r e a Y o k o h a m a A r t i s t : M a r i a n o P e n s o t t i ( P l a y w r i g h t, D i r e c t o r ) C o n t e n t s : T h i s w o

More information

Icarus. Spectral decomposition of asteroid Itokawa based on principal component analysis

Icarus. Spectral decomposition of asteroid Itokawa based on principal component analysis Icarus 299 (2018) 386 395 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Spectral decomposition of asteroid Itokawa based on principal component analysis

More information

Meteorites and mineral textures in meteorites. Tomoki Nakamura. Meteorites ~100 ton/yr Interplanetary dust ~40000 ton/yr.

Meteorites and mineral textures in meteorites. Tomoki Nakamura. Meteorites ~100 ton/yr Interplanetary dust ~40000 ton/yr. Meteorites ~100 ton/yr Interplanetary dust ~40000 ton/yr Meteorites and mineral textures in meteorites Tomoki Nakamura Челябинск Tohoku University Japan Barringer crater (Arizona USA) 1275m diameter and

More information

ETIKA V PROFESII PSYCHOLÓGA

ETIKA V PROFESII PSYCHOLÓGA P r a ž s k á v y s o k á š k o l a p s y c h o s o c i á l n í c h s t u d i í ETIKA V PROFESII PSYCHOLÓGA N a t á l i a S l o b o d n í k o v á v e d ú c i p r á c e : P h D r. M a r t i n S t r o u

More information

Mineralogy and crystallography of some Itokawa particles returned by the Hayabusa asteroidal sample return mission

Mineralogy and crystallography of some Itokawa particles returned by the Hayabusa asteroidal sample return mission Mikouchi et al. Earth, Planets and Space 2014, 66:82 FRONTIER LETTER Open Access Mineralogy and crystallography of some Itokawa particles returned by the Hayabusa asteroidal sample return mission Takashi

More information

Preliminary organic compound analysis of microparticles returned from Asteroid Itokawa by the Hayabusa mission

Preliminary organic compound analysis of microparticles returned from Asteroid Itokawa by the Hayabusa mission Geochemical Journal, Vol. 46, pp. 61 to 72, 2012 NOTE Preliminary organic compound analysis of microparticles returned from Asteroid 25143 Itokawa by the Hayabusa mission H. NARAOKA, 1 * H. MITA, 2 K.

More information

F O R SOCI AL WORK RESE ARCH

F O R SOCI AL WORK RESE ARCH 7 TH EUROPE AN CONFERENCE F O R SOCI AL WORK RESE ARCH C h a l l e n g e s i n s o c i a l w o r k r e s e a r c h c o n f l i c t s, b a r r i e r s a n d p o s s i b i l i t i e s i n r e l a t i o n

More information

Stardust and Hayabusa Missions. Mike Zolensky NASA JSC

Stardust and Hayabusa Missions. Mike Zolensky NASA JSC Stardust and Hayabusa Missions Mike Zolensky NASA JSC 150 km from nucleus ΔV= 6.1 km/s January 2, 2004 Wild 2 (81P) A Jupiter family comet captured into present orbit in 1973 after a 0.006 AU Jupiter encounter

More information

Extralunar Materials in Lunar Regolith

Extralunar Materials in Lunar Regolith ExtralunarMaterialsinLunarRegolith AWhitePaperSubmittedfortheNRCDecadalSurvey Authors: MarcFries,JetPropulsionLaboratory,PasadenaCA JohnArmstrong,WeberStateUniversity,OgdenUT JamesAshley,ArizonaStateUniversity,TempeAZ

More information

New insights on thermal properties of asteroids using IR interferometry

New insights on thermal properties of asteroids using IR interferometry New insights on thermal properties of asteroids using IR interferometry Alexis MATTER Marco Delbo Benoit Carry Sebastiano Ligori 1 PLAN Introduction Thermal properties of asteroids Physical parameters

More information

Introduction into cosmochemistry - what the meteorites can tell us

Introduction into cosmochemistry - what the meteorites can tell us Introduction into cosmochemistry - what the meteorites can tell us www.kosmochemie.de Wir erstaunen metallische und erdige Massen, welche der Außenwelt, den himmlischen Räumen angehören: betasten, wiegen,

More information

+Δη decreasing depth and width of 1-micron band. #Δη SUPPLEMENTARY INFORMATION. increasing depth and. width of 2-micron band. increasing depth and

+Δη decreasing depth and width of 1-micron band. #Δη SUPPLEMENTARY INFORMATION. increasing depth and. width of 2-micron band. increasing depth and increasing depth and width of 2-micron band +Δη decreasing depth and width of 1-micron band #Δη increasing depth and width of 1-micron band Supplementary Figure 1. Spectral trends within principal component

More information

. ffflffluary 7, 1855.

. ffflffluary 7, 1855. x B B - Y 8 B > ) - ( vv B ( v v v (B/ x< / Y 8 8 > [ x v 6 ) > ( - ) - x ( < v x { > v v q < 8 - - - 4 B ( v - / v x [ - - B v B --------- v v ( v < v v v q B v B B v?8 Y X $ v x B ( B B B B ) ( - v -

More information

The Tagish Lake Meteorite: A Possible Sample from a D-Type Asteroid

The Tagish Lake Meteorite: A Possible Sample from a D-Type Asteroid The Tagish Lake Meteorite: A Possible Sample from a D-Type Asteroid Takahiro Hiroi, 1 * Michael E. Zolensky, 2 Carle M. Pieters 1 1 Department of Geological Sciences, Brown University, Providence, RI 02912,

More information

Asteroids are arguably the most accessible remnants of building blocks

Asteroids are arguably the most accessible remnants of building blocks Establishing Asteroid Meteorite Links Edward A. Cloutis 1, Richard P. Binzel 2, and Michael J. Gaffey 3 1811-5209/14/0010-025$2.50 DOI: 10.2113/gselements.10.1.25 Asteroids are arguably the most accessible

More information

Student Guide to Moon 101

Student Guide to Moon 101 Student Guide to Moon 101 LINKS TO WEBSITES AND DOCUMENTS NECESSARY TO COMPLETE MOON 101 CAN BE FOUND AT: 1) Read the following articles: PART 1 - FORMATION OF THE MOON a) The Scientific Legacy of Apollo,

More information

P2IO SCIENTIFIC Life emergence conditions : P2IO R&D project

P2IO SCIENTIFIC Life emergence conditions : P2IO R&D project P2IO SCIENTIFIC P2IO SCIENTIFIC COUNCIL Life emergence conditions : P2IO R&D project Responsable du projet : Brunetto, Rosario, CNRS CR2 IAS-CNRS, UMR8617, Bat 121, Université Paris Sud, 91405 ORSAY, Cedex

More information

Robotic Lunar Exploration Scenario JAXA Plan

Robotic Lunar Exploration Scenario JAXA Plan Workshop May, 2006 Robotic Lunar Exploration Scenario JAXA Plan Tatsuaki HASHIMOTO JAXA 1 Question: What is Space Exploration? Answers: There are as many answers as the number of the people who answer

More information

Meteorite Analogs for Phobos and Deimos: Unraveling the Origin of the Martian Moons

Meteorite Analogs for Phobos and Deimos: Unraveling the Origin of the Martian Moons Meteorite Analogs for Phobos and Deimos: Unraveling the Origin of the Martian Moons P. Vernazza 1, F. Cipriani 1, C. Dukes 2, D. Fulvio 2, K. T. Howard 3, O. Witasse 1, R. Brunetto 4, G. Strazzulla 5,

More information

arxiv: v2 [astro-ph.ep] 30 Jan 2014

arxiv: v2 [astro-ph.ep] 30 Jan 2014 Scattered Light Correction of HAYABUSA/AMICA Data and Quantitative Spectral Comparisons of Itokawa arxiv:1401.7642v2 [astro-ph.ep] 30 Jan 2014 Masateru Ishiguro Department of Physics and Astronomy, Seoul

More information

Space weathering of asteroidal surfaces

Space weathering of asteroidal surfaces Space weathering of asteroidal surfaces Giovanni Strazzulla 1 & Rosario Brunetto 2 1 INAF Osservatorio Astrofisico di Catania, Italy gianni@oact.inaf.it 2 Institut d'astrophysique Spatiale, UMR 8617, Orsay,

More information

CARBONACEOUS CHONDRITES AND AQUEOUS ALTERATION

CARBONACEOUS CHONDRITES AND AQUEOUS ALTERATION CARBONACEOUS CHONDRITES AND AQUEOUS ALTERATION Discussion Summarizer: Ariel Deutsch Hiroi et al., 1996 INTRODUCTION The authors present a thermal metamorphism study by comparing the 0.7 µm, 3 µm, and UV

More information

International Workshop on Cutting-Edge Plasma Physics July Plasma Physics of the Lunar Surface

International Workshop on Cutting-Edge Plasma Physics July Plasma Physics of the Lunar Surface 2155-8 International Workshop on Cutting-Edge Plasma Physics 5-16 July 2010 Plasma Physics of Mihaly Horanyi Dept. of Physics University of Colorado at Boulder USA Plasma Physics of Mihaly Horanyi Colorado

More information

Joy of Science Experience the evolution of the Universe, Earth and Life

Joy of Science Experience the evolution of the Universe, Earth and Life Joy of Science Experience the evolution of the Universe, Earth and Life Review Introduction Main contents Quiz Unless otherwise noted, all pictures are taken from wikipedia.org Review 1 The presence of

More information

Pluto is not alone out there

Pluto is not alone out there Reading: Chapter 13, Sect. 13.1-13.4, Chapter 14, Sect. 14.1-14.2 Homework 9 - See course webpage later this week Exam 2 - Tuesday November 2 - in class - Physics 3 and 5 Practice exam, review sheets posted

More information

Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target JU3 from AKARI and Subaru Observations

Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target JU3 from AKARI and Subaru Observations PASJ: Publ. Astron. Soc. Japan 60, S399 S405, 2008 December 25 c 2008. Astronomical Society of Japan. Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target 162173 1999 JU3 from AKARI

More information

Hayabusa at Itokawa: first visit to a rubble pile asteroid, or

Hayabusa at Itokawa: first visit to a rubble pile asteroid, or Hayabusa at Itokawa: first visit to a rubble pile asteroid, or How do we know it s a rubble pile, and what does that mean? A. F. Cheng, O Barnouin-Jha, N. Hirata, H. Miyamoto, R. Nakamura, H. Yano and

More information

Lecture 31. Planetary Accretion the raw materials and the final compositions

Lecture 31. Planetary Accretion the raw materials and the final compositions Lecture 31 Planetary Accretion the raw materials and the final compositions Reading this week: White Ch 11 (sections 11.1-11.4) Today 1. Boundary conditions for Planetary Accretion Growth and Differentiation

More information

Framework for functional tree simulation applied to 'golden delicious' apple trees

Framework for functional tree simulation applied to 'golden delicious' apple trees Purdue University Purdue e-pubs Open Access Theses Theses and Dissertations Spring 2015 Framework for functional tree simulation applied to 'golden delicious' apple trees Marek Fiser Purdue University

More information

GLY August, Ms. Nelda Breedt. Fragment of extra-terrestrial material that strikes the surface of the Earth.

GLY August, Ms. Nelda Breedt. Fragment of extra-terrestrial material that strikes the surface of the Earth. Meteorite Impacts Ms. Nelda Breedt GLY 162 Environmental Geology 2 Meteorite Impacts Meteorite Fragment of extra-terrestrial material that strikes the surface of the Earth. Meteoroid Before hitting the

More information

Is there a magnetic field on asteroid (4) Vesta?

Is there a magnetic field on asteroid (4) Vesta? Is there a magnetic field on asteroid (4) Vesta? by Benoît Carry 1,2 in collaboration with: P. Vernazza (ESA/ESTEC), C. Dumas (ESO) & M. Fulchignoni (Obs. Paris) 1 European Southern Observatory 2 LESIA,Observatoire

More information

Vectors. Teaching Learning Point. Ç, where OP. l m n

Vectors. Teaching Learning Point. Ç, where OP. l m n Vectors 9 Teaching Learning Point l A quantity that has magnitude as well as direction is called is called a vector. l A directed line segment represents a vector and is denoted y AB Å or a Æ. l Position

More information

The Microscopic Properties Of Meteorites: Die Mikroskopic Beschaffenheit Der Meteoriten (Smithsonian Contributions To Astrophysics) By Gustav von

The Microscopic Properties Of Meteorites: Die Mikroskopic Beschaffenheit Der Meteoriten (Smithsonian Contributions To Astrophysics) By Gustav von The Microscopic Properties Of Meteorites: Die Mikroskopic Beschaffenheit Der Meteoriten (Smithsonian Contributions To Astrophysics) By Gustav von Tschermak ande. M. Wood, Translators, 1964: The microscopic

More information

Hayabusa's Adventure around a Tiny Asteroid Itokawa

Hayabusa's Adventure around a Tiny Asteroid Itokawa Hayabusa's Adventure around a Tiny Asteroid Itokawa COSPAR Capacity Building Workshop on Planetary Science July 23 - Aug. 3, 2007 Montevideo, Uruguay M. Yoshikawa, A. Fujiwara, J. Kawaguchi (JAXA) Hayabusa

More information

In class, Wednesday Oct 25. Please wait outside AT BACK until told to enter the room. Must write IN PEN. Non programming calculators allowed (and

In class, Wednesday Oct 25. Please wait outside AT BACK until told to enter the room. Must write IN PEN. Non programming calculators allowed (and Midterm material In class, Wednesday Oct 25. Please wait outside AT BACK until told to enter the room. Must write IN PEN. Non programming calculators allowed (and required) No notes or hats. Formulae provided

More information

Analysis of samples returned by space missions : Apollo, Genesis, Stardust, Marco Polo

Analysis of samples returned by space missions : Apollo, Genesis, Stardust, Marco Polo Analysis of samples returned by space missions : Apollo, Genesis, Stardust, Marco Polo Bernard Marty Centre de Recherches Pétrographiques et Géochimiques, UPR2300 CNRS Ecole Nationale Supérieure de Géologie

More information

! " # $! % & '! , ) ( + - (. ) ( ) * + / 0 1 2 3 0 / 4 5 / 6 0 ; 8 7 < = 7 > 8 7 8 9 : Œ Š ž P P h ˆ Š ˆ Œ ˆ Š ˆ Ž Ž Ý Ü Ý Ü Ý Ž Ý ê ç è ± ¹ ¼ ¹ ä ± ¹ w ç ¹ è ¼ è Œ ¹ ± ¹ è ¹ è ä ç w ¹ ã ¼ ¹ ä ¹ ¼ ¹ ±

More information

The Formation and Evolution of Ordinary Chondrite Parent Bodies

The Formation and Evolution of Ordinary Chondrite Parent Bodies The Formation and Evolution of Ordinary Chondrite Parent Bodies Pierre Vernazza Aix Marseille Université and Laboratoire d Astrophysique de Marseille Brigitte Zanda Muséum National d Histoire Naturelle

More information

Observing hydrated minerals on asteroids. Andy Rivkin (JHU/APL) JWST Workshop at DPS 10 October 2013 Denver CO

Observing hydrated minerals on asteroids. Andy Rivkin (JHU/APL) JWST Workshop at DPS 10 October 2013 Denver CO Observing hydrated minerals on asteroids Andy Rivkin (JHU/APL) JWST Workshop at DPS 10 October 2013 Denver CO Why asteroids? Asteroids represent leftover material not incorporated into the inner planets

More information

Hermes Experiment Opportunities

Hermes Experiment Opportunities Hermes Experiment Opportunities Kristen John (PI) and Marc Fries Astromaterials Research and Exploration Science (ARES) NASA Johnson Space Center Houston, TX Strata-1 and Hermes Strata-1 is a Class 1E

More information

Remote and surface X ray experiments of small bodies. T. Okada (JAXA, Japan)

Remote and surface X ray experiments of small bodies. T. Okada (JAXA, Japan) Remote and surface X ray experiments of small bodies T. Okada (JAXA, Japan) X X XRF C/D C chondrite Al/Si CIorCMorCV/CM CR S NEAR Hayabusa XRF XRD XRF Debye preparaion Raue non preparaion InstrumentaIon

More information

Name Topic 3 Free Response 2017

Name Topic 3 Free Response 2017 Name Topic 3 Free Response 2017 Base your answers to questions 1 and 2 on the graph and on your knowledge of Earth science. The graph shows planet equatorial diameters and planet mean distances from the

More information

(Received 04 May 2008; revision accepted 14 December 2008)

(Received 04 May 2008; revision accepted 14 December 2008) Meteoritics & Planetary Science 44, Nr 4, 521 530 (2009) Abstract available online at http://meteoritics.org Cooling rates of porphyritic olivine chondrules in the Semarkona (LL3.00) ordinary chondrite:

More information

Laboratory Simulations of Space Weathering Effects Giovanni Strazzulla INAF Osservatorio Astrofisico di Catania, Italy

Laboratory Simulations of Space Weathering Effects Giovanni Strazzulla INAF Osservatorio Astrofisico di Catania, Italy Laboratory Simulations of Space Weathering Effects Giovanni Strazzulla INAF Osservatorio Astrofisico di Catania, Italy gianni@oact.inaf.it http://web.ct.astro.it/weblab/ 1 NNNNNNNN kev-mev ions ELECTRONS

More information

CAPTEM. Curation and Analysis Planning Team for Extraterrestrial Materials. Kevin D. McKeegan Dept. of Earth, Planetary, and Space Sciences UCLA

CAPTEM. Curation and Analysis Planning Team for Extraterrestrial Materials. Kevin D. McKeegan Dept. of Earth, Planetary, and Space Sciences UCLA CAPTEM Curation and Analysis Planning Team for Extraterrestrial Materials Kevin D. McKeegan Dept. of Earth, Planetary, and Space Sciences UCLA Planetary Science Advisory Committee NASA HQ, Feb. 23, 2018

More information

Acid-susceptive material as a host phase of argon-rich noble gas in the carbonaceous chondrite Ningqiang

Acid-susceptive material as a host phase of argon-rich noble gas in the carbonaceous chondrite Ningqiang Meteoritics & Planetary Science 38, Nr 2, 243 250 (2003) Abstract available online at http://meteoritics.org Acid-susceptive material as a host phase of argon-rich noble gas in the carbonaceous chondrite

More information

Wed. Sept. 06, 2017 Reading:

Wed. Sept. 06, 2017 Reading: Wed. Sept. 06, 2017 Reading: For today: Wood Ch. 6 & 8 (Asteroids & Meteorites, Solar Nebula) For this Friday: Rozel et al. 2017 "Continental crust formation on early Earth controlled by intrusive magmatism."

More information

Volatiles (H, C, N, F, S, Cl) in the lunar mantle, crust, and regolith: What questions remain and where to go next?

Volatiles (H, C, N, F, S, Cl) in the lunar mantle, crust, and regolith: What questions remain and where to go next? Volatiles (H, C, N, F, S, Cl) in the lunar mantle, crust, and regolith: What questions remain and where to go next? Francis M. McCubbin & Charles K. Shearer Motivation behind this work 100, In Revision,

More information

http://eps.mcgill.ca/~courses/c201_winter/ http://eps.mcgill.ca/~courses/c201_winter/ Neutron Proton Nucleosynthesis neutron!! electron!+!proton!!=!!é!!+!h +!! t 1/2 =!12!minutes H + +!neutron!! Deuterium!(D)

More information

How Old is the Solar System?

How Old is the Solar System? How Old is the Solar System? Earth s crust is constantly changing due to volcanoes, erosion, and plate tectonics. So Earth rocks do not preserve a record of the early days of the Solar System. Instead,

More information

Analyzing the Chemical Composition and Classification of Miller Range 07273

Analyzing the Chemical Composition and Classification of Miller Range 07273 Alyssa Dolan Analyzing the Chemical Composition and Classification of Miller Range 07273 When small grains and debris that were present in the early solar system combine, they form meteoroids. Meteoroids

More information

arxiv: v1 [astro-ph] 16 Aug 2008

arxiv: v1 [astro-ph] 16 Aug 2008 accepted for publication in the ApJ Letter Rotation-Resolved Spectroscopy of a Very Young Asteroid, (1270) Datura arxiv:0808.2248v1 [astro-ph] 16 Aug 2008 Naruhisa Takato 1 Subaru Telescope, 650 North

More information

Scanning electron microscopical and cross sectional analysis of extraterrestrial carbonaceous nanoglobules

Scanning electron microscopical and cross sectional analysis of extraterrestrial carbonaceous nanoglobules Meteoritics & Planetary Science 43, Nr 5, 1 5 (2008) Abstract available online at http://meteoritics.org AUTHOR S PROOF Scanning electron microscopical and cross sectional analysis of extraterrestrial

More information

Microgravity Geology: A New Challenge for Human and Robotic Space Exploration

Microgravity Geology: A New Challenge for Human and Robotic Space Exploration Off Earth Mining Forum Microgravity Geology: A New Challenge for Human and Robotic Space Exploration February 20 th, 2013 Australian Centre for Space Engineering Research, University of New South Wales,

More information

Assignment 2. Due March 4, 2019

Assignment 2. Due March 4, 2019 Assignment 2 Due March 4, 2019 Show all work and turn in answers on separate pages, not on these pages. Circle your final answers for clarity. Be sure to show/explain all of your reasoning and that your

More information

Phone: Spoken languages: French and English. Citizenships: French & Belgian

Phone: Spoken languages: French and English. Citizenships: French & Belgian Pierre Haenecour Postdoctoral Research Fellow Earths in Other Solar Systems (EOS) team Lunar and Planetary Laboratory The University of Arizona 1629 E. University Blvd. Tucson, AZ 85721-0092 Citizenships:

More information

Impact process of boulders on the surface of asteroid Itokawa fragments from collisional disruption

Impact process of boulders on the surface of asteroid Itokawa fragments from collisional disruption Earth Planets Space, 60, 7 12, 2008 Impact process of boulders on the surface of asteroid 25143 Itokawa fragments from collisional disruption A. M. Nakamura 1, T. Michikami 2, N. Hirata 3, A. Fujiwara

More information

OSIRIS-REx. Asteroid Sample Return Mission. Dante S. Lauretta Deputy Principal Investigator

OSIRIS-REx. Asteroid Sample Return Mission. Dante S. Lauretta Deputy Principal Investigator OSIRIS-REx Asteroid Sample Return Mission Dante S. Lauretta Deputy Principal Investigator 2 OSIRIS-REX MISSION OBJECTIVES MAP ONE TO ONE WITH NASA KEY QUESTIONS NASA Key Questions How did life begin and

More information

New evidence for lunar basalt metasomatism by underlying regolith.

New evidence for lunar basalt metasomatism by underlying regolith. 1 2 3 4 5 New evidence for lunar basalt metasomatism by underlying regolith. John F. Pernet-Fisher* School of Earth, Atmospheric, and Environmental Sciences, University of Manchester, Manchester, M13 2PL,

More information

Where we are now. The Moon Chapters 8.2, 9. Topography. Outline

Where we are now. The Moon Chapters 8.2, 9. Topography. Outline Where we are now Introduction Little things - comets, asteroids, KBOs Slightly larger things - Moon Larger still - Terrestrial planets Really large - Jovian planets Jovian moons + Pluto Extrasolar Planets

More information

THE PLANETARY SCIENTIST'S COMPANION

THE PLANETARY SCIENTIST'S COMPANION THE PLANETARY SCIENTIST'S COMPANION Katharina Lodders Bruce Fegley, Jr. New York Oxford Oxford University Press 1998 Contents 1 Technical data Table 1.1 The Greek alphabet 1 Table 1.2 Prefixes used with

More information

Laboratory Analyses of Marco Polo Samples Ian Franchi

Laboratory Analyses of Marco Polo Samples Ian Franchi Laboratory Analyses of Marco Polo Samples Ian Franchi Planetary & Space Sciences Research Ins;tute, Open University, Milton Keynes, MK11 1HP, UK i.a.franchi@open.ac.uk Overview Principle Objec;ve of Marco

More information

Supporting Online Material for

Supporting Online Material for www.sciencemag.org/cgi/content/full/1142021/dc1 Supporting Online Material for Remnants of the Early Solar System Water Enriched in Heavy Oxygen Isotopes Naoya Sakamoto, Yusuke Seto, Shoichi Itoh, Kiyoshi

More information

But first... Asteroids. Asteroids... Lecture 3: Overview of Asteroids and Meteorites. Space junk...? Rosetta Stones...? or Harbingers of DOOM?

But first... Asteroids. Asteroids... Lecture 3: Overview of Asteroids and Meteorites. Space junk...? Rosetta Stones...? or Harbingers of DOOM? Lecture 3: Overview of Asteroids and Meteorites Astro 202 Prof. Jim Bell (jfb8@cornell.edu) Spring 2008 But first... A few words about Referencing in science writing... (see http://astrosun2.astro.cornell.edu/academics/courses/a202/referencing.html)

More information

Teachersʼ Guide. Creating Craters. Down to Earth KS3

Teachersʼ Guide. Creating Craters. Down to Earth KS3 Teachersʼ Guide Creating Craters Creating Craters! Creating Craters - Teachersʼ Guide - 2 Overview This lesson allows pupils to create impact craters in layered dry materials. Pupils can perform controlled

More information

Analyzing Next to Nothing

Analyzing Next to Nothing 1 of 5 posted April 26, 2000 Analyzing Next to Nothing Written by G. Jeffrey Taylor Hawai'i Institute of Geophysics and Planetology Analytical techniques have advanced so far that it is possible to slice

More information

The 2004 Las Campanas/Lowell Observatory campaign II. Surface properties of Hayabusa target Asteroid Itokawa inferred from Hapke modeling

The 2004 Las Campanas/Lowell Observatory campaign II. Surface properties of Hayabusa target Asteroid Itokawa inferred from Hapke modeling Earth Planets Space, 6, 49 59, 28 The 24 Las Campanas/Lowell Observatory campaign II. Surface properties of Hayabusa target Asteroid 25143 Itokawa inferred from Hapke modeling S. M. Lederer 1, D. L. Domingue

More information

AMHERST COLLEGE Department of Geology Geology 41: Environmental and Solid Earth Geophysics

AMHERST COLLEGE Department of Geology Geology 41: Environmental and Solid Earth Geophysics AMHERST COLLEGE Department of Geology Geology 41: Environmental and Solid Earth Geophysics Lab 1: Meteorites EQUIPMENT: notebook and pen only In this lab, we will examine thin sections and hand samples

More information

The Tagish Lake Meteorite: Clues to the Maturation of Organic Matter in the Early Solar System

The Tagish Lake Meteorite: Clues to the Maturation of Organic Matter in the Early Solar System The Tagish Lake Meteorite: Clues to the Maturation of Organic Matter in the Early Solar System Chris Herd Earth and Atmospheric Sciences Institute for Space Science, Exploration and Technology University

More information

Hayabusa2: Scientific importance of samples returned from C-type near-earth asteroid (162173) 1999 JU 3

Hayabusa2: Scientific importance of samples returned from C-type near-earth asteroid (162173) 1999 JU 3 Geochemical Journal, Vol. 48, pp. 571 to 587, 2014 doi:10.2343/geochemj.2.0350 Hayabusa2: Scientific importance of samples returned from C-type near-earth asteroid (162173) 1999 JU 3 S. TACHIBANA, 1 *

More information

http://eps.mcgill.ca/~courses/c220/ Nucleosynthesis neutron electron + proton = é + H + t 1/2 = 12 minutes H + + neutron Deuterium (D) 2 H + + neutrons Helium (He) 3 H + + neutrons Lithium (Li) From: W.S.

More information

Fundamentally distinct outcomes of asteroid collisional evolution: Itokawa and Eros

Fundamentally distinct outcomes of asteroid collisional evolution: Itokawa and Eros GEOPHYSICAL RESEARCH LETTERS, VOL. 34, L09201, doi:10.1029/2007gl029559, 2007 Fundamentally distinct outcomes of asteroid collisional evolution: Itokawa and Eros A. F. Cheng, 1 O. Barnouin-Jha, 1 N. Hirata,

More information

Astrodynamics Science about Itokawa, Gravity and Ephemeris

Astrodynamics Science about Itokawa, Gravity and Ephemeris AIAA/AAS Astrodynamics Specialist Conference and Exhibit 21-24 August 2006, Keystone, Colorado AIAA 2006-6658 Astrodynamics Science about Itokawa, Gravity and Ephemeris M. Yoshikawa *, H. Ikeda, H. Yano,

More information

Sampling Systems for Hayabusa and follow-on missions: Scientific Rationale, Operational Considerations, and Technological Challenges

Sampling Systems for Hayabusa and follow-on missions: Scientific Rationale, Operational Considerations, and Technological Challenges International Marco Polo Symposium and other Small Body Sample Return Missions Sampling Systems for Hayabusa and follow-on missions: Scientific Rationale, Operational Considerations, and Technological

More information

An Example file... log.txt

An Example file... log.txt # ' ' Start of fie & %$ " 1 - : 5? ;., B - ( * * B - ( * * F I / 0. )- +, * ( ) 8 8 7 /. 6 )- +, 5 5 3 2( 7 7 +, 6 6 9( 3 5( ) 7-0 +, => - +< ( ) )- +, 7 / +, 5 9 (. 6 )- 0 * D>. C )- +, (A :, C 0 )- +,

More information

Plasma and Dust-Plasma Environment at Bodies with and without Outgassing

Plasma and Dust-Plasma Environment at Bodies with and without Outgassing Plasma and Dust-Plasma Environment at Bodies with and without Outgassing Christine Hartzell University of Maryland 2018/10/29 Intro to Electrostatic Dust Motion Neutral PLasma E E Plasma Sheath λ D e -

More information

Lab 5: An Investigation of Meteorites Geology 202: Earth s Interior

Lab 5: An Investigation of Meteorites Geology 202: Earth s Interior Lab 5: An Investigation of Meteorites Geology 202: Earth s Interior Asteroids and Meteorites: What is the difference between asteroids and meteorites? Asteroids are rocky and metallic objects that orbit

More information

NEO Sample Return Mission

NEO Sample Return Mission Cannes, 5 Juin 2008 M.A. Barucci & M. Yoshikawa MARCO POLO NEO Sample Return Mission This mission, prepared by a joint European Japanese team, is supported by more than 450 confirmed scientists. Joint

More information

Composition of Near-Earth Asteroid (4179) Toutatis

Composition of Near-Earth Asteroid (4179) Toutatis "! #! $! %! &! '! (! )! *! "+! ""! "#! "$! "%! "&! "'! "(! ")! "*! #+! #"! ##! #$! Composition of Near-Earth Asteroid (4179) Toutatis Vishnu Reddy 1 Department of Space Studies, University of North Dakota,

More information

Redoing the Foundations of Decision Theory

Redoing the Foundations of Decision Theory Redoing the Foundations of Decision Theory Joe Halpern Cornell University Joint work with Larry Blume and David Easley Economics Cornell Redoing the Foundations of Decision Theory p. 1/21 Decision Making:

More information

Fleming County Schools Long Range Plan Teacher(s):

Fleming County Schools Long Range Plan Teacher(s): School Calendar Days Unit Title Standards August 2015 10 11 12 13 14 1-3 Get To Know You (2) Newton s Third Law of Motion (10) 17 18 19 20 21 4-8 Newton s Third Law of Motion 24 25 26 27 28 9-13 September

More information

Meteors. Meteors Comet dust particles entering our atmosphere and burning up from the friction. The Peekskill, NY Meteorite Fall.

Meteors. Meteors Comet dust particles entering our atmosphere and burning up from the friction. The Peekskill, NY Meteorite Fall. Meteors Meteors Comet dust particles entering our atmosphere and burning up from the friction. 2 Updated july 19, 2009 Every year about Nov. 18 the Earth goes through the path of an old comet. Meteorites

More information

Cohesive forces preventing rotational breakup of rubble pile asteroid (29075) 1950 DA

Cohesive forces preventing rotational breakup of rubble pile asteroid (29075) 1950 DA Cohesive forces preventing rotational breakup of rubble pile asteroid (29075) 1950 DA Ben Rozitis 1, Eric MacLennan 1 & Joshua P. Emery 1 1 Department of Earth and Planetary Sciences, University of Tennessee,

More information

(4) Meteorites: Remnants of Creation

(4) Meteorites: Remnants of Creation (4) Meteorites: Remnants of Creation Meteoroid: small piece of debris in space Meteor: space debris heated by friction as it plunges into the Earth s atmosphere Meteorite: Space debris that has reached

More information

Primitive Asteroids: Insight into the Formation and Evolution of the Solar System. Driss Takir USGS Astrogeology Science Center, Flagstaff, Arizona

Primitive Asteroids: Insight into the Formation and Evolution of the Solar System. Driss Takir USGS Astrogeology Science Center, Flagstaff, Arizona Primitive Asteroids: Insight into the Formation and Evolution of the Solar System Artist's impression of the asteroid belt. Image credit: NASA/JPL-Caltech Driss Takir USGS Astrogeology Science Center,

More information

CURRICULUM VITAE. Examination Specialization School/College Board/University

CURRICULUM VITAE. Examination Specialization School/College Board/University CURRICULUM VITAE Dr. Gagan Gupta Email: gagan.astro@gmail.com, gagangupta_17@yahoo.com Phone: 7589091005 TEACHING EXPERIENCE Guru Kashi University, Talwandi Sabo---- 2 nd September, 2011 to 4 th August,

More information

Mission Analysis of Sample Return from Jovian Trojan Asteroid by Solar Power Sail

Mission Analysis of Sample Return from Jovian Trojan Asteroid by Solar Power Sail Trans. JSASS Aerospace Tech. Japan Vol. 12, No. ists29, pp. Pk_43-Pk_50, 2014 Original Paper Mission Analysis of Sample Return from Jovian Trojan Asteroid by Solar Power Sail By Jun MATSUMOTO 1), Ryu FUNASE

More information