Direct Imaging Black Holes from LEO
Ref Bari | Update to Ben 07/22
Size
Weight
Power
Power
Cost
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
SEFD
USO
Data
Orbit
Quantization Efficiency: how much of the analog SNR is retained after digitization
Sub-milli arcsecond angular resolution:
Dual short and long baseline lengths
Rapid coverage of (u,v) plane
Decreased signal loss from LEO
Decreased radiation environment in LEO vs. MEO