Differences between revisions 1 and 2
Revision 1 as of 2015-08-14 20:54:08
Size: 638
Comment:
Revision 2 as of 2015-08-14 20:55:10
Size: 643
Comment:
Deletions are marked like this. Additions are marked like this.
Line 8: Line 8:
The Kuiper starts at approximately 30 AU and is constrained by observability. A 1500 kg/km^2^, 50 AU Dyson shell ( 7.46E9 km, 7e20 km^2^ ) uses 1e24 kg of ice and other materials; that is cut in half if we use [[IRFilter | front-side IR filtering ]]. The Kuiper starts at approximately 30 AU and is constrained by observability. A 1.5 g/m^2^, 50 AU Dyson shell ( 7.46E9 km, 7e20 km^2^ ) uses 1e24 kg of ice and other materials; that is cut in half if the shell uses [[IRfilter | front-side IR filtering ]].

KuiperBelt

The Structure of the Kuiper Belt: Size Distribution and Radial Extent, Brett Gladman et. al.

Bottom of page 1065: The disk mass in the observed region out to ≈ 60 AU is ≈ 0.1 Mearth (6e23 kg), only weakly dependent on the roll-over size and radial distribution.

The Kuiper starts at approximately 30 AU and is constrained by observability. A 1.5 g/m2, 50 AU Dyson shell ( 7.46E9 km, 7e20 km2 ) uses 1e24 kg of ice and other materials; that is cut in half if the shell uses front-side IR filtering.

KuiperBelt (last edited 2015-11-18 03:20:11 by KeithLofstrom)