Index
Note: Page numbers followed by f indicate figures and t indicate tables.
A
Age of rocky surfaces, impact craters
59–67
production function
59–61
electromagnetic process
19
Phobos and Deimos, dust from
230–231
Alpha-Proton X-ray Spectrometer (APXS)
260–261
Argon-argon (
40Ar/
39Ar) dating
53–55,
54f
Asteroid Impact and Deflection Assessment (AIDA)
265
Astronomical Unit (AU)
188
B
Basalts and brecciated basalts
105
block size-frequency distribution
67,
69f
measurements and techniques
67–69
size-frequency distribution
67,
69
Brecciated anorthosites
105
C
Carbon dioxide snow line
202
Charge-coupled devices (CCDs)
74–75
Chelyabinsk, dark portion of
131–132
Chondritic interplanetary dust particles
107
Christiansen features
77,
130
Citizen science projects
271
Continuous ejecta blanket
147
Cosmic Ray Exposure (CRE) age
56–57,
57f
Crater statistics programs
66–67
D
Dating surfaces, space weathering
134–136
D-class asteroid spectra
112
Decadal survey process
256
Depth and retention, regolith
160–162
Discontinuous ejecta blanket
147
Double Asteroid Redirection Test (DART)
265
Downslope movement, regolith
seismic shaking and regolith convection
174–177
E
remote sensing data from
96
Electromagnetic process
19
Electrostatic effects and levitation, regolith
180–183
Enstatite achondrites
103
European space agency
259,
262
Exploration
See also specific types
F
Fischer Tropsch–type reactions
129
G
Gamma-ray spectrometers (GRS)
81f,
82
Gamma-ray spectroscopy
81
Grains and space weathering
127–129
H
Hartmann plot (H-plot)
62,
64f
Hayabusa 2 mission
2,
263
Hayabusa X-ray measurements
130
data storage and processing
269–271
in situ resource utilization
266–268
Human Exploration and Operations Mission Directorate (HEOMD)
259–260
Hydrated interplanetary dust particles
107
I
production function
59–61
Impact ejecta blankets
147
Infrared Processing and Analysis Center (IPAC)
270
In situ resource utilization (ISRU)
266–268
Instruments, airless bodies
91t
International Space Exploration Coordination Group (ISECG)
266
Interplanetary dust particles (IDPs)
106–107
Irregular mare patches (IMP)
235–237
J
The Japanese Aerospace Exploration Agency (JAXA)
108
K
Keck/NASA Reflectance Experiment Laboratory (RELAB)
270
Keplerian orbital elements
188,
189f
Korea Pathfinder Lunar Orbiter (KPLO)
258,
259f
L
Lag deposits, regolith
160
Laser-induced breakdown spectroscopy (LIBS)
80
Layer silicate chondritic particles
107
Levitation of dust on asteroids
183
Low-albedo surfaces, space weathering on
129
Low-reflectance material (LRM)
213
Lunar Crater Observation and Sensing Satellite (LCROSS)
213–214
Lunar exploration
29,
29f
Lunar Reconnaissance Orbiter (LRO)
1,
34–35
M
Magnitudes, brightness in
84–86
Main belt comets (MBCs)
219
Mars Express (MEx) mission
41
Mars Reconnaissance Orbiter (MRO) mission
41,
221–222
Martian Moons Exploration (MMX) mission
261–262
surface composition
39–40
Mercury Dual Imaging System (MDIS)
83–84,
84f
Mercury Laser Altimeter (MLA)
89
Mercury Magnetospheric Orbiter (MMO)
260
Mercury Planetary Orbiter (MPO)
260
MINERVA-II-1A, -1B, -II
263
Mini-SAR instrument
34,
35f
remote sensing data from
96
space-weathering process
126
Moon Mineralogy Mapper (M
3)
34–35
Multiple Asteroids Rendezvous and in situ Survey Mission (MARS)
265–266
N
Narrow-angle camera (NAC)
110
Near-Infrared Spectrometer
263
NEAR Shoemaker mission
42–43
Neutron spectrometers (NS)
81f,
82
Neutron spectroscopy, volatile
206
New Frontiers missions
256
Nonchondritic interplanetary dust particles
107
O
Olivine chondritic particles
107
Optical Navigation Camera
263
Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx)
2,
263–264,
264f
P
retention of volatiles
209
Phobos Grunt spacecraft
262
Planetary Data System (PDS)
270
Potassium-Argon (K-Ar) dating
53–55
Primitive achondrites
103
Production function
59–61
Projects, citizen science
271
Pyroxene chondritic particles
107
R
Reflectance spectroscopy
74–79
spectral measurements
78–79
transmission spectra
76–77
seismic shaking and regolith convection
174–177
electrostatic effects and levitation
180–183
Relative plot (R-plot)
62,
64f
Remote elemental composition technique
81–82
craters, interpreting
97–98
interplanetary dust particles
106–107
Resonance, Mercury
14,
15f
Retention of volatile
209
magnitudes, brightness in
84–86
remote elemental composition technique
81–82
Rubble pile internal structures
157
Rubidium-87/strontium-87 (Rb-Sr) dating
51–52,
52f
Russian Phobos-Grunt mission
30
S
Samarium-147/neodymium-143 system (Sm-Nd)
55
Sample return mission
257
Shielding lunar swirls
242
Size-frequency distribution (SFD)
60–61
Sloan Digital Sky Survey data
270
Smart Lander for Investigating Moon (SLIM)
258
Solar system paradigms
32–33
sample return mission
257
on low-albedo surfaces
129
solar wind implantation and plasma interactions
132–134
Spectral energy distribution (SED)
77,
78f
magnitudes, brightness in
84–86
remote elemental composition technique
81–82
Spectroscopic measurements, volatile
206,
207f
Spectroscopy
74–75 See also specific types
Strategic knowledge gap (SKG)
257
Sulfur and space weathering
130–131
Surface composition, Mercury
39–40
T
Terminal Lunar Cataclysm (TLC)
36–37
Terrestrial analogs
96–98
Thermal fracturing, regolith
157–160
Thermal Infrared Imager
263
Time delay and integration (TDI) cameras
109–110
Transmission spectra
76–77
U
United States, planetary exploration
255–257
Uranium, thorium-lead (U, Th-Pb)
55,
56f
V
V class asteroid spectra
112,
114
W
Wavelengths, space weathering
130
Wide-angle camera (WAC)
110
Wien’s displacement law
74
X
Y
Z