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DTSTART;VALUE=DATE:20251215
DTEND;VALUE=DATE:20251216
DTSTAMP:20260613T120216
CREATED:20250105T220155Z
LAST-MODIFIED:20251212T222329Z
UID:10000057-1765756800-1765843199@spacecalendar.com
SUMMARY:Launch Atlas V 551 / Amazon Leo (LA-04)
DESCRIPTION:Scheduled for 03:35 UTC-5\, United Launch Alliance (ULA) rocket will take next batch of Amazon Leo (new name) satellites for internet system managed by Amazon subsidiary Kuiper Systems. ULA is a joint venture of Lockheed Martin Space and Boeing Defense\, Space & Security.
URL:https://spacecalendar.com/event/launch-atlas-v-551-amazon-leo-la-04/
LOCATION:SLC-41 (~28°N)\, Cape Canaveral SFS FL\, USA
CATEGORIES:Launch
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20251215
DTEND;VALUE=DATE:20251216
DTSTAMP:20260613T120216
CREATED:20250212T212421Z
LAST-MODIFIED:20251212T224922Z
UID:10000108-1765756800-1765843199@spacecalendar.com
SUMMARY:Launch Proton-M / Blok DM-03 / Elektro-L No.5
DESCRIPTION:Scheduled for 17:20 Kazakhstan Time. Meteorological satellites developed by NPO Lavochkin. Launch cost estimated at US$65M. Built at Khrunichev State Research and Production Space Center\, Moscow\, with 43\,000+ employees.
URL:https://spacecalendar.com/event/launch-proton-m-blok-dm-03-elektro-l-no-5/
LOCATION:Baikonur Cosmodrome\, ~46°N\, Kazakhstan
CATEGORIES:Launch
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BEGIN:VEVENT
DTSTART;VALUE=DATE:20251215
DTEND;VALUE=DATE:20251220
DTSTAMP:20260613T120216
CREATED:20251112T224015Z
LAST-MODIFIED:20251212T224053Z
UID:10000664-1765756800-1766188799@spacecalendar.com
SUMMARY:American Geophysical Union (AGU) 2025 Annual Meeting
DESCRIPTION:Features Session P046-To the Moon: A New Era of Lunar Science\, Session P030-Planetary Magnetism.
URL:https://spacecalendar.com/event/american-geophysical-union-agu-2025-annual-meeting2/
LOCATION:New Orleans LA\, USA
CATEGORIES:Meeting / Conference / Symposium
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BEGIN:VEVENT
DTSTART;VALUE=DATE:20251215
DTEND;VALUE=DATE:20251220
DTSTAMP:20260613T120216
CREATED:20251212T223545Z
LAST-MODIFIED:20251212T223545Z
UID:10000564-1765756800-1766188799@spacecalendar.com
SUMMARY:High-Resolution Spectroscopy for Exoplanet Atmospheres Workshop
DESCRIPTION:Over the next few decades\, the exoplanet community is poised to advance closer to answering a fundamental question about the universe and humanity’s place in it: Are we alone? High-resolution spectroscopy of exoplanets with the Extremely Large Telescopes (> 25 m) offers a unique opportunity to answer this question.  The high spectral resolutions and large apertures enable high signal-to-noise measurements of spectrally resolved lines of key atmospheric gases.  Current observational programs with 3 – 10 m class telescopes (e.g.\, TNG\,  ESO 3.6 m\, LDT\, CFHT\, Gemini N/S\, VLT\, Keck) and high resolution spectrographs (R>~15\,000\, e.g.\,  HARPS\, GIANO\, SPIRou\, ESPRESSO\, MAROON-X\, GHOST\, IGRINS\, CRIRES+) have and are continuing to reveal unique insights into the composition\, chemistry\, and climates of large gas giant planets.    \nHowever\, in order to maximize the science return from current instrumentation and the upcoming ELT’s\, there is a pressing need to train the next generation of scientists in this challenging but powerful observational method.  In particular\,  the pool of experts in this area within the US exoplanet community is rather small. Hence\, there is a pressing need to train US-based junior scientists in ground-based high spectral resolution observational and analysis techniques so that we maximize the science return from current and upcoming platforms.  \nThe goal of this week-long workshop is to provide sufficient background via lectures and hands-on activities such that attendees will be able to: \n\n\nOpen and read in pipeline processed data from a variety of US (e.g.\, IGRINS\, MAROON-X\, GHOST) and European-led (e.g\, ESPRESSO\, CRIRES+) instruments. \n\n\nApply common telluric removal methods like PCA\, SYSREM\, and forward modeling. \n\n\nPerform model template-data cross-correlation analyses to detect atmospheric gases in both the transmission and emission geometries. \n\n\nApply publicly available atmospheric retrieval tools combined with various CCF-to-log-likelihood mappings to obtain atmospheric parameter constraints. \n\n\nPlan and execute observations with a variety of instruments. \n\n\nThe workshop will be structured like the Sagan Summer Workshops\, with a mix of pedagogical lectures and hands-on activities\, as well as an opportunity for attendees to present their own work via daily poster sessions. 
URL:https://spacecalendar.com/event/high-resolution-spectroscopy-for-exoplanet-atmospheres-workshop/
LOCATION:Tempe AZ\, USA
CATEGORIES:Meeting / Conference / Symposium
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