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X-WR-CALDESC:The collecting of evidence is the most fundamental activity sc
 ientists engage in.  But what if the only evidence you have is visual and 
 indirect?  Until recently\, space science research relied entirely on visu
 al observations with no ability at all to directly make measurement\, coll
 ect data\, and examine phenomena. \n\nIn this module\, we look at how astr
 onomers can draw conclusions about the size\, distance\, composition\, and
  origins of planets and moons using only data collected at a distance.  Th
 rough an examination of the properties of solar system objects\, such as p
 lanets\, moon\, and comets\, participants will come away with a better und
 erstanding of how scientists explore these distant worlds and fragments\, 
 how they are classified\, and how our classification has evolved as new te
 chnology allows for more detailed observations.\n\nAppropriate for teachin
 g grade levels 3-12.\n\nRegistration deadline for Module 1 was August 15.
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X-WR-TIMEZONE:America/Los_Angeles
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TZNAME:PST
DTSTART:20191103T020000
TZOFFSETFROM:-0700
TZOFFSETTO:-0800
RDATE:20201101T020000
RDATE:20211107T020000
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DTSTART:20200308T020000
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RDATE:20210314T020000
RDATE:20220313T020000
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BEGIN:VEVENT
UID:af6a16c7-96a6-49b7-9622-883dd0f53c4c
DTSTAMP:20260404T162525Z
DESCRIPTION:The collecting of evidence is the most fundamental activity sci
 entists engage in.  But what if the only evidence you have is visual and i
 ndirect?  Until recently\, space science research relied entirely on visua
 l observations with no ability at all to directly make measurement\, colle
 ct data\, and examine phenomena. \n\nIn this module\, we look at how astro
 nomers can draw conclusions about the size\, distance\, composition\, and 
 origins of planets and moons using only data collected at a distance.  Thr
 ough an examination of the properties of solar system objects\, such as pl
 anets\, moon\, and comets\, participants will come away with a better unde
 rstanding of how scientists explore these distant worlds and fragments\, h
 ow they are classified\, and how our classification has evolved as new tec
 hnology allows for more detailed observations.\n\nAppropriate for teaching
  grade levels 3-12.\n\nRegistration deadline for Module 1 was August 15.
DTSTART;TZID=America/Los_Angeles:20200915T160000
DTEND;TZID=America/Los_Angeles:20200915T170000
LOCATION:Online Webinar Series
SUMMARY:TLC Online Astronomy Institute: Module 1 Exploring the Solar System
END:VEVENT
END:VCALENDAR