'50 au' presentation slideshows

Credit: ESO

836 views • 80 slides

FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: PROBING INITIAL CONDITIONS AND OUTCOMES WITH E-ELT

FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: PROBING INITIAL CONDITIONS AND OUTCOMES WITH E-ELT. Michael R. Meyer Institute for Astronomy Department of Physics (and many, many, others) HARMONI Early Science, Oxford, 2 July, 2015.

304 views • 30 slides

Dave Meyer Northwestern University

Optical/UV Absorption Line Observations of Small-Scale Interstellar Structure. Dave Meyer Northwestern University. UV Absorption-Line Measurements of Interstellar Abundances. GHRS: Cardelli & Meyer (1997). STIS: Cartledge, Meyer, & Lauroesch (2003).

312 views • 22 slides

Asteroids and Kuiper Belt Objects

Asteroids and Kuiper Belt Objects. Know about Pluto Know about the Asteroids Know about Comets Comprehend the Oort Cloud and Kuiper Belt. The Discovery of Pluto. Percival Lowell predicted the existence of an additional planet in 1905

368 views • 14 slides

Gas in Transitional Disks

Gas in Transitional Disks. Sean Brittain Clemson University, Clemson, SC, USA Joan Najita National Optical Astronomy Observatory, Tucson, AZ, USA. 5 th Planet Formation Workshop. Interpretation of the SED. Interpretation of the SED. Malfait et al. 1998. Gas in Transitional Disks.

265 views • 13 slides

Does the Kuiper Belt have an edge?

Does the Kuiper Belt have an edge?. Ming-Chang Liu. Introduction. Kuiper Belt, a thick band of small bodies beyond the orbit of Neptune, has an extended range from 30 AU to 50 AU.

217 views • 9 slides