Near-Ultraviolet and Visible Spectroscopy of HAYABUSA Spacecraft Re-Entry

Abe Shinsuke; Fujita Kazuhisa; Kakinami Yoshihiro; Iiyama Ohmi; Kurosaki Hirohisa; Shoemaker Michael A.; Shiba Yasuo; Ueda Masayoshi; Suzuki Masaharu

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Near-Ultraviolet and Visible Spectroscopy of HAYABUSA Spacecraft Re-Entry

机译：HAYABUSA航天器重新进入的近紫外和可见光谱

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HAYABUSAisthefirstspacecraftevertolandonandliftofffromanycelestialbodyotherthanthemoon.Themission,whichreturnedasteroidsamplestotheEarthwhileovercomingvarioustechnicalhurdles,endedon2010June13,withtheplannedatmosphericre-entry.Inordertosafelydeliverthesamplereturncapsule,theHAYABUSAspacecraftendedits7-yearjourneyinabrilliant``artificialfireball''overtheAustraliandesert.Spectroscopicobservationwascarriedoutinthenear-ultravioletandvisiblewavelengthsbetween3000?…and7500?…at3a€“20?…resolution.Approximately100atomiclinessuchasFei,Mgi,Nai,Ali,CrI,Mni,Nii,Tii,Lii,Zni,Oi,andNiwereidentifiedfromthespacecraft.ExoticatomssuchasCui,Moi,XeiandHgiwerealsodetected.AstrongLiiline(6708?…)ataheightof$$sim$$55kmoriginatedfromtheonboardLi-Ionbatteries.TheFeOmoleculebandsataheightof$$sim$$63kmwereprobablyformedinthewakeofthespacecraft.Theeffectiveexcitationtemperatureasdeterminedfromtheatomiclinesvariedfrom4500Kto6000K.TheobservednumberdensityofFeiwasabout10timesmoreabundantthanMgiafterthespacecraftexplosion.N$$_{2}^{+}$$($$1^-$$)bandsfromashocklayerandCNvioletbandsfromthesamplereturncapsule'sablatingheatshieldweredominantmolecularbandsinthenear-ultravioletregionof3000a€“4000?….OH($$A$$a€“$$X$$)bandwaslikelytoexistaround3092?….AstrongshocklayerfromtheHAYABUSAspacecraftwasrapidlyformedatheightsbetween93kmand83km,whichwasconfirmedbydetectionofN$$_{2}^{+}$$($$1^-$$)bandswithavibrationtemperatureof$$sim$$13000K.Gray-bodytemperatureofthecapsuleataheightof$$sim$$42kmwasestimatedtobe$$sim$$2437Kwhichismatchedtoatheoreticalprediction.ThefinalmessageoftheHAYABUSAspacecraftanditssamplereturncapsulearediscussedthroughourspectroscopy.

机译：HAYABUSAisthefirstspacecraftevertolandonandliftofffromanycelestialbodyotherthanthemoon.Themission，whichreturnedasteroidsamplestotheEarthwhileovercomingvarioustechnicalhurdles，endedon2010June13，withtheplannedatmosphericre-entry.Inordertosafelydeliverthesamplereturncapsule，theHAYABUSAspacecraftendedits7-yearjourneyinabrilliant``artificialfireball''overtheAustraliandesert.Spectroscopicobservationwascarriedoutinthenear-ultravioletandvisiblewavelengthsbetween3000？... and7500？... at3a€“20？... resolution.Approximately100atomiclinessuchasFei，MGI，奈，阿里，国际广播电台， MNI，哥哥，TII，吕叔湘，Zni，爱，andNiwereidentifiedfromthespacecraft.ExoticatomssuchasCui，莫伊，XeiandHgiwerealsodetected.AstrongLiiline（6708？...）ataheightof $$ SIM $$ 55kmoriginatedfromtheonboardLi-Ionbatteries.TheFeOmoleculebandsataheightof $$ SIM $$ 63kmwereprobablyformedinthewakeofthespacecraft.Theeffectiveexcitationtemperatureasdeterminedfromtheatomiclinesvariedfrom4500Kto6000K.TheobservednumberdensityofFeiwasabout10timesmoreabundantthanMgiafterthespacecraftexplosi N。$$ _ {2} ^ {+} $$（$$ 1 ^-$$）的带是来自冲击层的，而样品返回胶囊的消融热屏蔽的聚醚分子带的聚氯乙烯带则在3000-4000欧元附近。OH。（$$ A $ a $$$$ X $$）可能在3092年左右存在一个带？……。来自HAYABUS航天器的强震层迅速形成了93公里至83公里之间的高度，通过检测到N $$ _ {2} ^ {+} $$（$$ ^-$$）个带确认的温度，测得的温度，模拟的温度是$ sim于$$ K到$ 3000的$$ sim {$$ ^^-$$}，证实了$ 437到$ 437的温度。通过光谱学讨论了HAYABUS航天器的最终消息及其样品返回舱。

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《PASJ: Publications of the Astronomical Society of Japan》 |2011年第5期|共页
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Abe Shinsuke; Fujita Kazuhisa; Kakinami Yoshihiro; Iiyama Ohmi; Kurosaki Hirohisa; Shoemaker Michael A.; Shiba Yasuo; Ueda Masayoshi; Suzuki Masaharu;
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1. Near-ultraviolet and visible spectroscopy of HAYABUSA spacecraft re-entry [J] . Abe S., Fujita K., Kakinami Y., PASJ: Publications of the Astronomical Society of Japan . 2011,第5期

机译：HAYABUSA航天器再进入的近紫外和可见光谱
2. Near-Ultraviolet and Visible Spectroscopy of HAYABUSA Spacecraft Re-Entry [J] . Abe Shinsuke, Fujita Kazuhisa, Kakinami Yoshihiro, PASJ: Publications of the Astronomical Society of Japan . 2011,第5期

机译：HAYABUSA航天器重新进入的近紫外和可见光谱
3. Fragmentation of the HAYABUSA spacecraft on re-entry [J] . Watanabe J.-I., Ohkawa T., Sato M., PASJ: Publications of the Astronomical Society of Japan . 2011,第5期

机译：HAYABUSA航天器的碎片再次进入
4. Visible and Near Infrared Spectroscopy of Hayabusa Re-entry using semi-autonomous tracking [C] . Timothy J. Mclntyre, Razmi Khan, Troy N. Eichmann, AIAA aerospace sciences meeting including the new horizons forum and aerospace exposition . 2012

机译：半自动跟踪的of鸟折返的可见和近红外光谱
5. A STUDY TO DETERMINE THE BASIC NEEDS OF MK'S UPON RE-ENTRY TO THE UNITED STATES AND TO DEFINE AND DESCRIBE A RE-ENTRY PROGRAM DESIGNED TO MEET THE NEEDS (MISSIONARY CHILDREN, THIRD CULTURE, INTERNATIONAL). [D] . SCHULZ, THOMAS NEIL. 1985

机译：确定MK再次进入美国的基本需求并确定和描述旨在满足需求的再进入计划的研究（传教儿童，第三文化，国际）。
6. From the CoverPNAS Plus: Space environment of an asteroid preserved on micrograins returned by the Hayabusa spacecraft [O] . Eizo Nakamura, Akio Makishima, Takuya Moriguti, 2012

机译：来自CoverPNAS Plus：Hayabusa航天器返回的保留在微颗粒上的小行星的空间环境
7. Near-Ultraviolet and Visible Spectroscopy of HAYABUSA Spacecraft Re-entry [O] . Shinsuke Abe, Kazuhisa Fujita, Yoshihiro Kakinami, 2011

机译：HaYaBUsa航天器重返入口的近紫外和可见光谱
8. Visible and near-ultraviolet spectroscopy at Thule AFB (76.5 N) from January 28 - February 15, 1988 [R] . Mount, G. H., Sanders, R. W., Jakoubek, R. O., 1988

机译：1988年1月28日至2月15日Thule aFB（76.5 N）的可见光和近紫外光谱

Near-Ultraviolet and Visible Spectroscopy of HAYABUSA Spacecraft Re-Entry

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