BEGIN:VCALENDAR VERSION:2.0 PRODID:-//chikkutakku.com//RDFCal 1.0//EN X-WR-CALDESC:GoogleカレンダーやiCalendar形式情報を共有シェ アしましょう。近所のイベントから全国のイベントま で今日のイベント検索やスケジュールを決めるならち っくたっく X-WR-CALNAME:ちっくたっく X-WR-TIMEZONE:UTC BEGIN:VEVENT SUMMARY:Ulibarri et al. (2023) Icarus 391\, 115319 DTSTART;VALUE=DATE-TIME:20260427T070000Z DTEND;VALUE=DATE-TIME:20260427T080000Z UID:275670177133 DESCRIPTION:文献:Ulibarri et al. (2023) Icarus 391\, 115319題目:Hy pervelocity Impact Ionization of Amino-Acid-Laden Dust: First Direct Measu rements and Implications for Instrument Capabilities and Prebiotic Chemis try要旨:The detection and characterization of organic molecules in cos mic dust are central to understanding prebiotic chemistry and habitabilit y across the solar system. In particular\, amino acids serve as key biom arkers due to their fundamental role in terrestrial biology and their pre sence in abiotic extraterrestrial materials. However\, the survivability and detectability of amino acids during hypervelocity impacts\, typical o f interplanetary dust particle (IDP) collisions and impact ionization mas s spectrometer (I2MS) detections\, remain poorly constrained.In this stud y\, we present the first direct laboratory measurements of hypervelocity impact ionization of amino-acid-laden dust grains. Aluminum particles coa ted with histidine and arginine were accelerated at velocities ranging fr om ~1 to 52 km/s and analyzed using a prototype I2MS analogous to flight instruments such as IDEX and SUDA. Time-of-flight mass spectra demonstrat e that both intact parent molecules and characteristic fragment ions surv ive impact and remain detectable at velocities up to at least ~6-7 km/s .These results provide critical validation for the capability of I2MS ins truments to identify organic compounds in situ during space missions and suggest that amino acids can persist under relevant hypervelocity conditi ons. Consequently\, continuous bombardment by IDPs may represent a viable mechanism for the delivery and redistribution of prebiotic molecules acr oss planetary environments. This work establishes a new experimental fram ework for assessing organic survivability and enhances confidence in futu re astrobiological investigations of dust populations throughout the sola r system.話者:Zachary Ernest Ulibarri (Cornell Univ.)言語:英語 LOCATION: END:VEVENT END:VCALENDAR