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by | Dec 24, 2013 | Daily Paper Summaries | 2 comments

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About Jessica Donaldson

I am a graduate student in the Astronomy department at the University of Maryland, College Park. My research interests include exoplanets and planet formation in circumstellar disks. Currently I work on observations of gas poor debris disks, the dusty remnants of the last stages of planet formation. I work with Aki Roberge at NASA Goddard Space Flight Center using mostly space-based observatories to characterize the dust.

Related posts:

The strength of planet formation: planets found in dense star clusters Testing the Titius-Bode law on exoplanets A super-precise super-Earth: measuring a planet’s radius to within 120 km Professional Photometry with a Consumer Camera

2 Comments

  1. Sam Grunblatt on January 4, 2014 at 11:52 am

    Just wanted to point out that saying this planet has no atmosphere at all may not be true-some believe that it may be possible the planet harbors clouds of silicate material, essentially giving it an atmosphere of vaporized rock.

    Reply
  2. Jonathan Slavin on January 10, 2014 at 12:39 pm

    one little errata: sin(0) = 0 — for “perfectly aligned” I think you mean that the orbit axis is 90 degrees from our line of sight so i = 90 and sin(i) = 1.

    Reply

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