Skip to main content
SearchLogin or Signup

Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches

Published onMay 31, 2019
Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches
·

Abstract

The brightness and spatial distribution of warm (~200K) dust structures located within a few AU We motivate and identify here the main instrumental / observational advances required to gain further insights into the origins of exozodiacal dust clouds and better understand their impact on planetary habitability and habitability searches.

The full text of this article is only available in PDF format:



Comments
0
comment

No comments here