_________________________________________________________________________________ Lesson Summary Students create a planet using a computer game and change features of the planet to increase or decrease the planet’s tem

First Page		Document Content
Date: 2013-06-17 16:04:29 Planetary science Thermodynamics Infrared Mars Black-body radiation Greenhouse effect Stefan–Boltzmann law Climate of Mars Water vapor Astronomy Atmospheric sciences Electromagnetic radiation		_________________________________________________________________________________ Lesson Summary Students create a planet using a computer game and change features of the planet to increase or decrease the planet’s tem Add to Reading List Source URL: lasp.colorado.edu Download Document from Source Website File Size: 4,12 MB Share Document on Facebook

	The Climate of Early Mars Robin D. Wordsworth1,2 1 arXiv:1606.02813v1 [astro-ph.EP] 9 Jun 2016 DocID: 1tUQu - View Document
	Transient Bright “Halos” on the South Polar Residual Cap of Mars: Implications for Mass-Balance 500 m • • DocID: 1rdsO - View Document
	Where glacier lovers and sheep collide a tale about my participation in the Karthaus Glaciology summer school 2013 “Earth or Mars?” DocID: 1q9sO - View Document
	JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 108, NO. E8, 5089, doi:2002JE001921, 2003 An assessment of the global, seasonal, and interannual spacecraft record of Martian climate in the thermal infrared Junjun Liu and DocID: 1pMFm - View Document
	MAVEN Science Results Bruce Jakosky LASP / University of Colorado MEPAG meeting, 3 March 2016 NOTE ADDED BY JPL WEBMASTER: This content has not been approved or adopted by, NASA, JPL, or the California Institute of Techn DocID: 1okGe - View Document