OCAMS: The OSIRIS-REx Camera Suite
Space Sci Rev (2018) 214:26
https://doi.org/10.1007/s11214-017-0460-7
OCAMS: The OSIRIS-REx Camera Suite
B. Rizk1 · C. Drouet d’Aubigny1 · D. Golish1 · C. Fellows1 · C. Merrill2 · P. Smith1 ·
M.S. Walker3 · J.E. Hendershot4 · J. Hancock5 · S.H. Bailey1,2 · D.N. DellaGiustina1 ·
D.S. Lauretta1 · R. Tanner1 · M. Williams1 · K. Harshman1 · M. Fitzgibbon1 ·
W. Verts6 · J. Chen7 · T. Connors2 · D. Hamara1 · A. Dowd8 · A. Lowman6 · M. Dubin6 ·
R. Burt5 · M. Whiteley5 · M. Watson5 · T. McMahon2 · M. Ward2 · D. Booher9 ·
M. Read1 · B. Williams2 · M. Hunten1 · E. Little9 · T. Saltzman1 · D. Alfred2 ·
S. O’Dougherty6 · M. Walthall9 · K. Kenagy2 · S. Peterson1 · B. Crowther5,10 ·
M.L. Perry1 · C. See1 · S. Selznick1 · C. Sauve2 · M. Beiser9 · W. Black6 ·
R.N. Pfisterer11 · A. Lancaster9 · S. Oliver2 · C. Oquest1 · D. Crowley1 · C. Morgan1 ·
C. Castle12 · R. Dominguez2 · M. Sullivan2
Received: 22 March 2017 / Accepted: 13 December 2017
© The Author(s) 2017. This article is published with open access at Springerlink.com
Abstract The OSIRIS-REx Camera Suite (OCAMS) will acquire images essential to collecting a sample from the surface of Bennu. During proximity operations, these images will
document the presence of satellites and plumes, record spin state, enable an accurate model
of the asteroid’s shape, and identify any surface hazards. They will confirm the presence of
sampleable regolith on the surface, observe the sampling event itself, and image the sample
head in order to verify its readiness to be stowed. They will document Bennu’s history as
an example of early solar system material, as a microgravity body with a planetesimal sizeOSIRIS-REx
Edited by Dante Lauretta and Christopher T. Russell
B B. Rizk
1
Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
2
Steward Observatory, University of Arizona, Tucson, AZ, USA
3
Goddard Space Flight Center, Greenbelt, MD, USA
4
Ball Aerospace, Greenbelt, MD, USA
5
Space Dynamics Laboratory, Utah State University Foundation, Logan, UT, USA
6
College of Optical Sciences, University of Arizona, Tucson, AZ, USA
7
Baja Technology LLC, Tucson, AZ, USA
8
Lithe Technology LLC, Tucson, AZ, USA
9
Raytheon Missile Systems, Tucson, AZ, USA
10
Synopsys Optical Solutions Group, Pasadena, CA, USA
11
Photon Engineering, L.L.C., Tucson, AZ, USA
12
Hofstadter Analytical, Tucson, AZ, USA
26
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B. Rizk et al.
scale, and as a carbonaceous object. OCAMS is fitted with three cameras. The MapCam
will record color images of Bennu as a point source on approach to the asteroid in order to
connect Bennu’s ground-based point-source observational record to later higher-resolution
surface spectral imaging. The SamCam will document the sample site before, during, and
after it is disturbed by the sample mechanism. The PolyCam, using its focus mechanism,
will observe the sample site at sub-centimeter resolutions, revealing surface texture and
morphology. While their imaging requirements divide naturally between the three cameras,
they preserve a strong degree of functional overlap. OCAMS and the other spacecraft instruments will allow the OSIRIS-REx mission to collect a sample from a microgravity body on
the same visit during which it was first optically acquired from long range, a useful capability as humanity reaches out to explore near-Earth, Main-Belt and Jupiter Trojan asteroids.
Keywords OSIRIS-REx · Bennu · Asteroid · Imaging · Sample return · OCAMS
Acronyms
AAM
APID
A/D, ADC
ATLO
C&DH
CCD
CCM
CDS
CM
CPU
CTE
DA
DN
DPU
DRM
DTCI
DTM
ECAS
EPER
EQM
F/
FITS
FM
FOV
FPGA
FRED
FSW
FWHM
GNC
GSFC
HGA
IFOV
IP
ISO
Asteroid Approach Maneuver
Application Process Identification
Analog-to-Digital Conversion
Assembly, Test, and Launch Operations
Command and Data Handling
Charge-Coupled Device
Camera Control Module
Correlated Double Sampling
Configuration Management
Computer Processing Unit
Coefficient of Thermal Expansion
Detector Assembly
Data Number
Data Processing Unit
Design Reference Mission
Data Telemetry Command Interface
Digital Terrain Model
Eight-Color Asteroid Survey
Extended-Pixel Edge Response
Engineering Qualification Model
F-Stop or F-number
Flexible Image Transport System
Flight Model
Field of View
Field-Programmable Gate Array
Fred Optical Engineering Software
Flight Software
Full-Width-at-Half-Max
Guidance Navigation and Control
Goddard Space Flight Center
High Gain Antenna
Instantaneous Field of View
Intellectual Property
International Standards Organization
OCAMS: The OSIRIS-REx Camera Suite
L1
LED
LGA
LIDAR
LPL
LSF
LVDS
LVPS
MapCam
MDR
MGA
MHD
MTF
NASA
NFPO
NFT
NIR
NIST
OCAMS
OLA
OSIRIS-REx
OST
OTES
OVIRS
Pan
PAPL
PCB
PIL
PSNIT
PolyCam
PRT
QTH
REXIS
RMS
ROI
RTS
RWA
SamCam
S/C
S/N, SNR
SDRAM
SPI
SRC
TAG
TAGCAMS
TAGSAM
Ti 6Al-4V
TID
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26
Lens 1
Light-Emitting Diode
Low Gain Antenna
Light Detection and Ranging
Lunar and Planetary Laboratory
Line-Spread Function
Low-Voltage Differential Signaling
Low-Voltage Power Supply
Mapping Camera
Minimum Detectable Radiance
Medium Gain Antenna
Motor/Heater Interface/Driver
Modulation Transfer Function
National Aeronautics and Space Administration
New Frontiers Program Office
Natural Feature Tracking
Near-Infrared
National Institute of Standards & Technology
OSIRIS-REx Camera Suite
OSIRIS-REx Laser Altimeter
Origins, Spectral Interpretation, Resource Identification, Security–Regolith
Explorer
Optical Support Tube
OSIRIS-REx Thermal Emission Spectrometer
OSIRIS-REx Visible and InfraRed Spectrometer
Panchromatic
Project-Approved Parts List
Parts Control Board
Parts Identification List
Point Source Normalized Irradiance Transmittance
Polyfunctional Camera
Platinum Resistance Thermometer
Quartz-Tungsten-Halogen
Regolith X-ray Imaging Spectrometer
Root-Mean-Square
Region of Interest
Random Telegraph Signal
Reaction Wheel Assembly
Sample Acquisition Verification Camera
Spacecraft
Signal-to-Noise Ratio
Synchronous Dynamic Random Access Memory
Serial Peripheral Interface
Sample Return Capsule
Touch And Go
Touch And Go Camera System
Touch And Go Sample Acquisition Maneuver
Titanium Alloy (Titanium, 6% Aluminum, 4% Vanadium)
Total Ionization Dose
26
TVAC
UA
UUT
UV
VML
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B. Rizk et al.
Thermal Vacuum
University of Arizona
Unit-Under-Test
Ultraviolet
Virtual Machine Language
1 Introduction
The sample-return mission of the Origins, Spectral Interpretation, Resource Identification
and Security–Regolith Explorer (OSIRIS-REx) must thoroughly characterize the near-Earth
asteroid 101955 Bennu before being able to acquire a sample from a scientifically interesting location on its surface with minimal risk, either to the spacecraft or to mission success (Ajluni et al. 2015; Beshore et al. 2015; Lauretta 2015, 2016; Bierhaus et al. 2018;
Lauretta et al. 2018). In addition, the mission team will map Bennu’s global properties,
characterize its geologic and dynamical history, document the morphology and chemistry
of the sample site, and determine Ben (...truncated)