In this proposal, we seek to apply the optical/thermal method to the measurement of the diameters and albedos of a large sample of Near Earth Objects (NEOs). Whereas main-belt asteroids have been studied in large numbers, principally using thermal detections from the IRAS satellite, relatively few thermal observations of NEOs have been secured. This program capitalizes on our access to large telescopes and imaging thermal IR detectors in pursuit of the definitive set of albedo data on the NEOs
Space missions to near-Earth objects (NEOs) are being planned at all major space agencies, and recen...
The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) reactivation mission has complet...
The metal content of asteroids is of great interest, not only for theories of their origins and the ...
More than 12000 Near-Earth Objects (NEOs) have been discovered over the past few decades and current...
More than 12000 Near-Earth Objects (NEOs) have been discovered over the past few decades and current...
While the physical characterization of near-Earth objects (NEOs) is progressing at a much slower rat...
While the physical characterization of near-Earth objects (NEOs) is progressing at a much slower rat...
The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) spacecraft has been conducting a...
Near Earth Objects (NEOs) are fragments of remnant primitive bodies that date from the era of Solar ...
Near-Earth objects (NEOs) are small solar system bodies whose orbits bring them close to the Earth’s...
Thermal infrared observations are the most effective way to measure asteroid diameter and albedo for...
With the NEOWISE portion of the Wide-field Infrared Survey Explorer (WISE) project, we have carried ...
The majority of Near Earth Objects (NEOs) originated in collisions between bodies in the main astero...
Near-Earth objects (NEOs) are small solar system bodies whose orbits bring them close to the Earth’s...
We review the physical principles on which asteroid thermal models are based and their application i...
Space missions to near-Earth objects (NEOs) are being planned at all major space agencies, and recen...
The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) reactivation mission has complet...
The metal content of asteroids is of great interest, not only for theories of their origins and the ...
More than 12000 Near-Earth Objects (NEOs) have been discovered over the past few decades and current...
More than 12000 Near-Earth Objects (NEOs) have been discovered over the past few decades and current...
While the physical characterization of near-Earth objects (NEOs) is progressing at a much slower rat...
While the physical characterization of near-Earth objects (NEOs) is progressing at a much slower rat...
The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) spacecraft has been conducting a...
Near Earth Objects (NEOs) are fragments of remnant primitive bodies that date from the era of Solar ...
Near-Earth objects (NEOs) are small solar system bodies whose orbits bring them close to the Earth’s...
Thermal infrared observations are the most effective way to measure asteroid diameter and albedo for...
With the NEOWISE portion of the Wide-field Infrared Survey Explorer (WISE) project, we have carried ...
The majority of Near Earth Objects (NEOs) originated in collisions between bodies in the main astero...
Near-Earth objects (NEOs) are small solar system bodies whose orbits bring them close to the Earth’s...
We review the physical principles on which asteroid thermal models are based and their application i...
Space missions to near-Earth objects (NEOs) are being planned at all major space agencies, and recen...
The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) reactivation mission has complet...
The metal content of asteroids is of great interest, not only for theories of their origins and the ...