INITIAL PERFORMANCE OF THE NEOWISE REACTIVATION MISSION

Первые результаты работы миссии реактивации NEOWISE
Peter Eisenhardt, Carl J. Grillmair, R. M. Cutri, J. Davy Kirkpatrick, J. W. Fowler, H. McCallon, S. Wheelock, Lin Yan, R. Beck, Frank J. Masci, S. B. Fajardo‐Acosta, Emily L. Rice, T. Grav, J. M. Bauer, Amy Mainzer, E. L. Wright, M. Papin, M. Wittman, R. Stevenson, J. Masiero, J. Dailey, T. Conrow, D. Royer, I. Heinrichsen, M. Kendall, Beth Fabinsky, Paul Clarkson, Christopher R. Gelino, F. Liu, C. Nugent, Thomas Curran Ryan, Pedro Sevilla, S. Sonnett, D. B. Thompson, D. Wiemer
2014-08-12

NEOWISE reactivation missioninfrared sky surveynear-Earth asteroidsradiometric diameters and albedosthermal emission
NASA's Wide-field Infrared Survey Explorer ( WISE ) spacecraft has been brought out of hibernation and has resumed surveying the sky at 3.4 and 4.6 μm. The scientific objectives of the NEOWISE reactivation mission are to detect, track, and characterize near-Earth asteroids and comets. The search for minor planets resumed on 2013 December 23, and the first new near-Earth object (NEO) was discovered 6 days later. As an infrared survey, NEOWISE detects asteroids based on their thermal emission and is equally sensitive to high and low albedo objects; consequently, NEOWISE -discovered NEOs tend to be large and dark. Over the course of its three-year mission, NEOWISE will determine radiometrically derived diameters and albedos for ∼2000 NEOs and tens of thousands of Main Belt asteroids. The 32 months of hibernation have had no significant effect on the mission's performance. Image quality, sensitivity, photometric and astrometric accuracy, completeness, and the rate of minor planet detections are all essentially unchanged from the prime mission's post-cryogenic phase.
1
Because NEOWISE detects thermal emission and is similarly sensitive to high- and low-albedo objects, its discovered NEOs tend to be large and dark.
2
Image quality, sensitivity, photometric and astrometric accuracy, completeness, and minor-planet detection rates remained essentially unchanged from the prime mission’s post-cryogenic phase.
3
NASA’s WISE spacecraft successfully resumed sky surveys at 3.4 and 4.6 μm after 32 months of hibernation.
4
Over three years, NEOWISE is expected to derive radiometric diameters and albedos for approximately 2,000 NEOs and tens of thousands of Main Belt asteroids.
5
The reactivated NEOWISE mission searches for, tracks, and characterizes near-Earth asteroids and comets, with its first new NEO discovered six days after searching resumed.

near-Earth asteroids and comets observed by the NEOWISE reactivation mission

their detection, tracking, characterization, and radiometrically derived diameters and albedos

Publication Details
Publication Date
2014-08-12
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Authors
Peter Eisenhardt
Carl J. Grillmair
R. M. Cutri
J. Davy Kirkpatrick
J. W. Fowler
H. McCallon
S. Wheelock
Lin Yan
R. Beck
Frank J. Masci
S. B. Fajardo‐Acosta
Emily L. Rice
T. Grav
J. M. Bauer
Amy Mainzer
E. L. Wright
M. Papin
M. Wittman
R. Stevenson
J. Masiero
J. Dailey
T. Conrow
D. Royer
I. Heinrichsen
M. Kendall
Beth Fabinsky
Paul Clarkson
Christopher R. Gelino
F. Liu
C. Nugent
Thomas Curran Ryan
Pedro Sevilla
S. Sonnett
D. B. Thompson
D. Wiemer
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