Index


Index

1 billion-light-year grid
Extragalactic Coordinate Grids
1 million-light-year grid
Extragalactic Coordinate Grids
1,000-light-year grid
Earth's Radio Sphere | Sun-Centered Coordinate Grids
1-light-month grid
The Farthest Man-Made Objects | Sun-Centered Coordinate Grids
1-light-year grid
The Oort Cloud Shows | Sun-Centered Coordinate Grids
10 million-light-year grid
Extragalactic Coordinate Grids
10,000-light-year grid
OB Associations Are in | Sun-Centered Coordinate Grids
10-light-year grid
The Nearest Stars Are | Sun-Centered Coordinate Grids
100 million-light-year grid
Extragalactic Coordinate Grids
100,000-light-year grid
Extragalactic Coordinate Grids
100-light-year grid
Sun-Centered Coordinate Grids
20 billion-light-year grid
Extragalactic Coordinate Grids
2dF Survey
2dF Galaxy Survey
galaxies
Galaxy Surveys | 2dF Galaxy Survey
quasars
Quasar Surveys | 2dF Quasar Survey
2MASS Galaxy Catalog
2MASS Galaxy Catalog
2MASS proximity factor
The Proximity Factor | Data Variables
Abell Galaxy Clusters
Abell Galaxy Clusters and
absolute magnitude
Intrinsic Brightnesses
active data group
Partiview's User Interface
all-sky survey
atomic hydrogen
Atomic Hydrogen Survey
carbon monoxide
Carbon Monoxide All-Sky Survey
far-infrared
Far Infrared Survey
gamma-ray
Gamma-Ray All-Sky Survey
hydrogen-alpha
Hydrogen-Alpha All-Sky Survey
IRAS composite
IRAS Composite All-Sky Survey
microwave
Microwave (WMAP) All-Sky Survey
two-micron
Two Micron (2MASS) All-Sky
visible
Visible All-Sky Survey | Visible All-Sky Survey
alpha command
Brightening the Lines | The Band of the
Alpha Slider
Partiview's User Interface | The Band of the
alternate star names
Alternate Star Names
Andromeda Galaxy
We Are a Member | Size of Our Star | Galaxy Image | Galaxies | Appendix: Light-Travel Time and
apparent magnitude
Stellar Brightness
astronomical unit
Appendix: Constants and Units
atomic hydrogen all-sky survey
Atomic Hydrogen Survey
att Button
Partiview's User Interface
B-V color
Color Is Derived from
Back Button
Partiview's User Interface
Big Bang
The Cosmic Microwave Background | The Cosmic Microwave Background | Microwave (WMAP) All-Sky Survey
bow shock
The Orion Nebula Model
Box Toggle Button
Partiview's User Interface
brown dwarf
Dwarf Catalog
carbon monoxide all-sky survey
Carbon Monoxide All-Sky Survey
celestial coordinates
Celestial Coordinates Resemble Earth's | Celestial Coordinates Sphere | Celestial Coordinates
censize command
Changing the Point of
Censize Slider
Partiview's User Interface | Changing the Point of
center command
Seeing Uncertainty | The Sun Is 26,000
clip command
Adjust the Clipping Planes | We Are a Member
clipbox command
Local Large-Scale Structure
clipping planes
Adjust the Clipping Planes | We Are a Member
cment command
Changing Their Color
COBE mission
Microwave (WMAP) All-Sky Survey
command
alpha
Brightening the Lines | The Band of the
censize
Changing the Point of
center
Seeing Uncertainty | The Sun Is 26,000
clip
Adjust the Clipping Planes | We Are a Member
clipbox
Local Large-Scale Structure
cment
Changing Their Color
datavar
Stellar Data Variables
every
A Random Subset
jump
The Nearest Stars
lsize
We Are a Member
lum const
Setting the Stars to
lum datavar
Setting the Stars to
only=
Galactic Census
see
Intrinsically Bright Stars Lie | Threshold the Stars
see all
Stellar Distances Are Determined
textcment
Changing the Label Color | Exoplanetary Systems
thresh
Stellar Brightness | Seeing Only the Nearest | Galactic Census
Command Line
Partiview's User Interface
Console Window
Partiview's User Interface
constellations
Constellations | Constellation Connectivity Lines | Constellations
coordinate system
celestial
Celestial Coordinates Resemble Earth's | Celestial Coordinates Sphere | Celestial Coordinates
ecliptic
Ecliptic Coordinates are Based | Ecliptic Coordinates are Based | Ecliptic Coordinates Sphere
equatorial
see celestial
Galactic
Galactic Coordinates Trace the | Galactic Coordinates Sphere | Galactic Coordinates
Cosmic Background Explorer
Microwave (WMAP) All-Sky Survey
cosmic microwave background
The Cosmic Microwave Background | Edge of the Observable | Microwave (WMAP) All-Sky Survey
origin
Origin of the CMB
temperature
The Cosmic Microwave Background
dark energy
The Distance Scale
data group list
Extragalactic Atlas
Extragalactic Atlas Overview
Milky Way Atlas
Milky Way Atlas Overview
data groups
100kly
Extragalactic Coordinate Grids
100ly
Sun-Centered Coordinate Grids
100Mly
Extragalactic Coordinate Grids
10kly
OB Associations Are in | Sun-Centered Coordinate Grids
10ly
The Nearest Stars Are | Sun-Centered Coordinate Grids
10Mly
Extragalactic Coordinate Grids
1Gly
Extragalactic Coordinate Grids
1kly
Earth's Radio Sphere | Sun-Centered Coordinate Grids
1lmo
The Farthest Man-Made Objects | Sun-Centered Coordinate Grids
1ly
The Oort Cloud Shows | Sun-Centered Coordinate Grids
1Mly
Extragalactic Coordinate Grids
20Gly
Extragalactic Coordinate Grids
2dFgals
Galaxy Surveys | 2dF Galaxy Survey
2dFQSOs
Quasar Surveys | 2dF Quasar Survey
2MASS
2MASS Galaxy Catalog
Abell
Abell Galaxy Clusters and
altLbl
Alternate Star Names
bar
Our Barred Galaxy | Galactic Bar
bulge
The Galactic Bulge | The Galactic Bulge
constel
Constellations | Constellation Connectivity Lines | Constellations
dso
Deep-Sky Images
dwarfs
Dwarf Catalog
eclip
Ecliptic Coordinates are Based | Ecliptic Coordinates Sphere
err
Distance Uncertainty | The Stellar Distance Uncertainty
expl
Exoplanetary Systems | Extrasolar Planets
Extragalactic Atlas
Extragalactic Data Groups
list
Extragalactic Atlas Overview
galac
Galactic Coordinates Trace the | Galactic Coordinates Sphere | Galactic Coordinates
galaxy
The Galactic Disk | Galaxy Image | Galaxy Image
galGrid
Galaxy Coordinate Grid
gc
Globular Clusters Are Mostly | Globular Clusters | Globular Star Clusters
h2
HII Regions | HII Regions
halo
The Galactic Halo | The Galactic Halo | Milky Way Halo
IRASc
IRAS Composite All-Sky Survey
isoDensity
Tully's Smoothed Density Surfaces
lgrp
We Are a Member | Local Group of Galaxies
local
The Local Universe | Local Galaxies
Milky Way Atlas
Milky Way Data Groups
list
Milky Way Atlas Overview
mw2MASS
Two Micron (2MASS) All-Sky
mwCO
Carbon Monoxide All-Sky Survey
mwFIR
Far Infrared Survey
mwGamma
Gamma-Ray All-Sky Survey
mwH
Atomic Hydrogen Survey
mwHa
Hydrogen-Alpha All-Sky Survey
mwVis
The Band of the | Visible All-Sky Survey | Visible All-Sky Survey
nearstars
Nearby Stars
ob
OB Associations | OB Associations
oc
Open Clusters Are Found | Open Star Clusters | Open Star Clusters
oort
The Oort Cloud Shows | Oort Cloud Sphere
oricl
Orion Nebula Star Cluster
orineb
The Orion Nebula Model
pn
Planetary Nebulae
probes
The Farthest Man-Made Objects | Spacecraft Trajectories
pul
Pulsars Are Spinning Neutron | Pulsars
radec
Celestial Coordinates Resemble Earth's | Earth's Radio Sphere | Celestial Coordinates Sphere | Celestial Coordinates
SloanGals
Galaxy Surveys | Sloan Galaxy Survey
SloanQSOs
Quasar Surveys | Sloan Quasar Survey
sloanstars
Sloan Stars
snr
Supernova Remnants Are the | Supernova Remnants
solsys
The Solar System | Planetary Orbits
starorbits
Stellar Orbits
stars
AMNH Stars | AMNH Fixed Stars
Tully
Local Large-Scale Structure | Tully's Nearby Galaxies | Tully Galaxy Catalog
wmap
Edge of the Observable | Microwave (WMAP) All-Sky Survey
data variables
Stellar Data Variables
datavar command
Stellar Data Variables
declination
Celestial Coordinates Resemble Earth's
deep-sky images
Deep-Sky Images
Digital Universe
configure
Customizing the Digital Universe
customize
Customizing the Digital Universe
discussion group
Getting Help
files
Digital Universe Files
help
Getting Help
installing
Installing the Digital Universe
license
Digital Universe License
listserve
Getting Help
starting
Launching the Milky Way | Digital Universe Files
distance
light-travel time
Appendix: Light-Travel Time and
light-year
Appendix: Light-Travel Time and
parallax
Appendix: Parallax and Distance
parsec
Appendix: Parallax and Distance | Appendix: Constants and Units
redshift
Appendix: Redshift and Distance
distance uncertainty
Distance Uncertainty
dwarf objects
Dwarf Catalog
Earth's radio signals
Earth's Radio Sphere
ecliptic
Ecliptic Coordinates are Based
ecliptic coordinates
Ecliptic Coordinates are Based | Ecliptic Coordinates Sphere
electromagnetic spectrum
Appendix: Electromagnetic Spectrum
elliptical galaxy
Galaxies | Data Variables
emission nebula
The Orion Nebula Model
every command
A Random Subset
Extragalactic Atlas
1 billion-light-year grid
Extragalactic Coordinate Grids
1 million-light-year grid
Extragalactic Coordinate Grids
10 million-light-year grid
Extragalactic Coordinate Grids
100 million-light-year grid
Extragalactic Coordinate Grids
100,000-light-year grid
Extragalactic Coordinate Grids
20 billion-light-year grid
Extragalactic Coordinate Grids
2dF Survey
galaxies
Galaxy Surveys | 2dF Galaxy Survey
quasars
Quasar Surveys | 2dF Quasar Survey
2MASS Galaxy Catalog
2MASS Galaxy Catalog
Abell Galaxy Clusters
Abell Galaxy Clusters and
celestial coordinates
Celestial Coordinates
constellations
Constellations
data group list
Extragalactic Atlas Overview
Galactic coordinates
Galactic Coordinates
local galaxies
The Local Universe | Local Galaxies
microwave all-sky survey
Edge of the Observable | Microwave (WMAP) All-Sky Survey
Milky Way
halo
Milky Way Halo
image
Galaxy Image
optimizing
Optimizing the Extragalactic Atlas
overview
Extragalactic Atlas Overview
Sloan Digital Sky Survey
galaxies
Galaxy Surveys | Sloan Galaxy Survey
quasars
Quasar Surveys | Sloan Quasar Survey
stars
Sloan Stars
stars data group
AMNH Fixed Stars
Tully density surface
Tully's Smoothed Density Surfaces
Tully galaxy catalog
Local Large-Scale Structure | Tully's Nearby Galaxies | Tully Galaxy Catalog
visible all-sky survey
Visible All-Sky Survey
extrasolar planets
Exoplanetary Systems | Extrasolar Planets
far-infrared all-sky survey
Far Infrared Survey
Feed Button
Partiview's User Interface
files
*.bat
Digital Universe Files
*.cf
Customizing the Digital Universe
*.cmap
Digital Universe Files
*.command
Digital Universe Files
*.label
Digital Universe Files
*.obj
Digital Universe Files
*.sgi
Digital Universe Files
*.sh
Digital Universe Files
*.speck
Digital Universe Files
color map
Digital Universe Files
configure
Customizing the Digital Universe
data
Digital Universe Files
image
Digital Universe Files
label
Digital Universe Files
start script
Digital Universe Files
finger of god effect
Seeing Uncertainty | Radial Stretching
flight mode
active
Moving Off the Point
changing
Changing the Flight Mode | Using the Keyboard to
Fly
Flight Modes | Moving Off the Point
Orbit
Flight Modes | Moving Off the Point
Rotate
Flight Modes | Using the Keyboard to
Translate
Flight Modes | Translate Flight Mode
Flight Mode Menu
Partiview's User Interface
flight path
control
att Button
Partiview's User Interface
Flight Path Slider
Partiview's User Interface
Frame Controls
Partiview's User Interface
Path Button
Partiview's User Interface
Play Button
Partiview's User Interface
loading
Partiview's User Interface
playing
Partiview's User Interface
Flight Path Slider
Partiview's User Interface
flight scale
linear
Flight Scale
logarithmic
Flight Scale
Fly Flight Mode
Flight Modes | Moving Off the Point
FOV Slider
Partiview's User Interface | What Do Other Data
Galactic coordinates
Galactic Coordinates Trace the | Galactic Coordinates Sphere | Galactic Coordinates
galactic star clusters
see open star clusters
galaxy
cluster
Cosmological Structure Formation
interaction
Our Nearest Neighbor
redshift
Appendix: Redshift and Distance
supercluster
Cosmological Structure Formation
types
Galaxies | Data Variables
Galaxy grid
Galaxy Coordinate Grid
galaxy superclusters
Abell Galaxy Clusters and
gamma-ray all-sky survey
Gamma-Ray All-Sky Survey
gamma-ray light
Appendix: Electromagnetic Spectrum
globular star cluster
age
Open Clusters Are Younger
globular star clusters
Globular Clusters Are Mostly | Globular Clusters | Globular Star Clusters
grids
extragalactic
1 billion-light-year
Extragalactic Coordinate Grids
1 million-light-year
Extragalactic Coordinate Grids
10 million-light-year
Extragalactic Coordinate Grids
100 million-light-year
Extragalactic Coordinate Grids
100,000-light-year
Extragalactic Coordinate Grids
20 billion-light-year grid
Extragalactic Coordinate Grids
Galaxy
Galaxy Coordinate Grid
Sun-centered
1,000-light-year
Sun-Centered Coordinate Grids
1-light-month
Sun-Centered Coordinate Grids
1-light-year
Sun-Centered Coordinate Grids
10,000-light-year
Sun-Centered Coordinate Grids
10-light-year
Sun-Centered Coordinate Grids
100-light-year
Sun-Centered Coordinate Grids
Group Buttons
Partiview's User Interface
Groups Menu
Partiview's User Interface
help
Getting Help
HII regions
HII Regions | HII Regions | The Orion Nebula Model
Hipparchus
Stellar Brightness
Home Button
Partiview's User Interface
Hubble's Law
Appendix: Redshift and Distance
Hubble, Edwin
Size of Our Star | Galaxy Image | Galaxies | The Magellanic Clouds | Data Variables
Hyades star cluster
Distance Uncertainty
hydrogen-alpha all-sky survey
Hydrogen-Alpha All-Sky Survey
infrared light
Why Use Infrared Telescopes? | Appendix: Electromagnetic Spectrum
installation
Installing the Digital Universe
IRAS composite all-sky survey
IRAS Composite All-Sky Survey
irregular galaxy
Galaxies | Data Variables
jump command
The Nearest Stars
Kelvin
Appendix: Constants and Units
L dwarf
Dwarf Catalog
Label Toggle Button
Partiview's User Interface
Labelmin Slider
Partiview's User Interface
Labelsize Slider
Partiview's User Interface
Large Magellanic Cloud
The Magellanic Clouds
large-scale structure
Galaxies
light-day
The Farthest Man-Made Objects | Appendix: Light-Travel Time and
light-hour
Appendix: Light-Travel Time and
light-month
Appendix: Light-Travel Time and | Appendix: Light-Travel Time and
light-second
Appendix: Light-Travel Time and
light-travel time
Appendix: Light-Travel Time and
light-week
Appendix: Light-Travel Time and
light-year
Appendix: Light-Travel Time and | Appendix: Constants and Units
linear flight scale
Flight Scale
local galaxies
The Local Universe | Local Galaxies
Local Group
We Are a Member | Local Group of Galaxies | Galaxies | The Local Group | Galaxy Clusters and Superclusters | Data Variables
Local Supercluster
Galaxy Clusters and Superclusters
logarithmic flight scale
Flight Scale
look-back time
Appendix: Redshift and Distance
lsize command
We Are a Member
lum const command
Setting the Stars to
lum datavar command
Setting the Stars to
Macintosh mouse
Mouse Controls
menu
Flight Mode
Partiview's User Interface
Groups
Partiview's User Interface
More
Partiview's User Interface
Slider
Partiview's User Interface
Messier, Charles
Deep-Sky Images
micron
Appendix: Constants and Units
microwave all-sky survey
Edge of the Observable | Microwave (WMAP) All-Sky Survey
microwave light
Appendix: Electromagnetic Spectrum
Milky Way
The Milky Way Atlas
bar
Our Barred Galaxy | Galactic Bar
bulge
The Galactic Bulge | The Galactic Bulge
disk component
The Galactic Disk
halo
The Galactic Halo | The Galactic Halo | Milky Way Halo
image
The Galactic Disk | Galaxy Image | Galaxy Image
nucleus
The Galactic Center
spherical component
The Spherical Component
spiral arms
Astronomers Use HII Regions
Milky Way Atlas
1,000-light-year grid
Earth's Radio Sphere | Sun-Centered Coordinate Grids
1-light-month grid
The Farthest Man-Made Objects | Sun-Centered Coordinate Grids
1-light-year grid
The Oort Cloud Shows | Sun-Centered Coordinate Grids
10,000-light-year grid
OB Associations Are in | Sun-Centered Coordinate Grids
10-light-year grid
The Nearest Stars Are | Sun-Centered Coordinate Grids
100-light-year grid
Sun-Centered Coordinate Grids
alternate star names
Alternate Star Names
atomic hydrogen all-sky survey
Atomic Hydrogen Survey
carbon monoxide all-sky survey
Carbon Monoxide All-Sky Survey
celestial coordinates
Celestial Coordinates Resemble Earth's | Celestial Coordinates Sphere
constellations
Constellations | Constellation Connectivity Lines
data group list
Milky Way Atlas Overview
deep-sky images
Deep-Sky Images
dwarf objects
Dwarf Catalog
ecliptic coordinates
Ecliptic Coordinates are Based | Ecliptic Coordinates Sphere
extrasolar planets
Exoplanetary Systems | Extrasolar Planets
far-infrared all-sky survey
Far Infrared Survey
Galactic coordinates
Galactic Coordinates Trace the | Galactic Coordinates Sphere
Galaxy grid
Galaxy Coordinate Grid
gamma-ray all-sky survey
Gamma-Ray All-Sky Survey
globular star clusters
Globular Clusters Are Mostly | Globular Clusters | Globular Star Clusters
HII regions
HII Regions | HII Regions
hydrogen-alpha all-sky survey
Hydrogen-Alpha All-Sky Survey
IRAS composite all-sky survey
IRAS Composite All-Sky Survey
Local Group
We Are a Member | Local Group of Galaxies
Milky Way
bar
Our Barred Galaxy | Galactic Bar
bulge
The Galactic Bulge | The Galactic Bulge
halo
The Galactic Halo | The Galactic Halo
image
The Galactic Disk | Galaxy Image
Nearby Stars
Nearby Stars
OB associations
OB Associations | OB Associations
Oort cloud
The Oort Cloud Shows | Oort Cloud Sphere
open star clusters
Open Clusters Are Found | Open Star Clusters | Open Star Clusters
optimizing
Optimizing the Milky Way
Orion Nebula
The Orion Nebula Model
Orion Nebula star cluster
Orion Nebula Star Cluster
overview
Milky Way Atlas Overview
planetary nebulae
Planetary Nebulae
planetary orbits
The Solar System | Planetary Orbits
pulsars
Pulsars Are Spinning Neutron | Pulsars
radio sphere
Earth's Radio Sphere
spacecraft trajectories
The Farthest Man-Made Objects | Spacecraft Trajectories
stars data group
AMNH Stars
stellar distance uncertainty
Distance Uncertainty | The Stellar Distance Uncertainty
stellar orbits
Stellar Orbits
supernova remnants
Supernova Remnants Are the | Supernova Remnants
two-micron all-sky survey
Two Micron (2MASS) All-Sky
visible all-sky survey
The Band of the | Visible All-Sky Survey
More Menu
Partiview's User Interface
mouse controls
Mouse Controls
Group Buttons
Partiview's User Interface
navigation
Flight Modes
mw.cf file
Customizing the Digital Universe | Save Your Changes
navigation
Flight Modes
Nearby Stars
Nearby Stars
nebula
emission
The Orion Nebula Model
OB associations
OB Associations | OB Associations
observable Universe
The Cosmic Microwave Background
only= command
Galactic Census
Oort cloud
The Oort Cloud Shows | Oort Cloud Sphere
open star cluster
age
Open Clusters Are Younger
open star clusters
Open Clusters Are Found | Open Star Clusters | Open Star Clusters
Orbit Flight Mode
Flight Modes | Moving Off the Point
Orion Nebula
The Orion Nebula Model
Orion Nebula star cluster
Orion Nebula Star Cluster
parallax
photometric
Photometric Parallax
trigonometric
Stellar Distances Are Determined | Appendix: Parallax and Distance
parsec
Appendix: Parallax and Distance | Appendix: Constants and Units
Partiview
command
alpha
Brightening the Lines | The Band of the
censize
Changing the Point of
center
Seeing Uncertainty | The Sun Is 26,000
clip
Adjust the Clipping Planes | We Are a Member
clipbox
Local Large-Scale Structure
cment
Changing Their Color
datavar
Stellar Data Variables
entering
Partiview's User Interface
every
A Random Subset
jump
The Nearest Stars
lsize
We Are a Member
lum const
Setting the Stars to
lum datavar
Setting the Stars to
only=
Galactic Census
see
Intrinsically Bright Stars Lie | Threshold the Stars
see all
Stellar Distances Are Determined
textcment
Changing the Label Color | Exoplanetary Systems
thresh
Stellar Brightness | Seeing Only the Nearest | Galactic Census
Command Line
Partiview's User Interface
Console Window
Partiview's User Interface
flight modes
Flight Modes
flight path controls
att Button
Partiview's User Interface
Flight Path Slider
Partiview's User Interface
Frame Controls
Partiview's User Interface
Path Button
Partiview's User Interface
Play Button
Partiview's User Interface
Group Buttons
Partiview's User Interface
Home Button
Partiview's User Interface
menu
Flight Mode
Partiview's User Interface
Groups
Partiview's User Interface
More
Partiview's User Interface
Slider
Partiview's User Interface
navigation
Learning to Fly Partiview
position reset
The Nearest Stars Are
slider
Alpha
Partiview's User Interface | The Band of the
Censize
Partiview's User Interface | Changing the Point of
Flight Path
Partiview's User Interface
FOV
Partiview's User Interface | What Do Other Data
Labelmin
Partiview's User Interface
Labelsize
Partiview's User Interface
Polysides
Partiview's User Interface
Polysize
Partiview's User Interface
range
Partiview's User Interface
Scale Button
Partiview's User Interface
Slum
Partiview's User Interface | Exoplanetary Systems
Speed
Partiview's User Interface
time controls
Back Button
Partiview's User Interface
Feed Button
Partiview's User Interface
Reference Time Display
Partiview's User Interface
Speed Slider
Partiview's User Interface
Speed Toggle Button
Partiview's User Interface
Time Control Buttons
Partiview's User Interface
Time Dial
Partiview's User Interface
Time Display
Partiview's User Interface
Trip Button
Partiview's User Interface
toggle button
Box
Partiview's User Interface
Label
Partiview's User Interface
Point
Partiview's User Interface
Polygon
Partiview's User Interface | Viewing the Solar System
Speed
Partiview's User Interface
Texture
Partiview's User Interface
user interface
Partiview's User Interface
Path Button
Partiview's User Interface
photometric parallax
Photometric Parallax
Pioneer spacecraft
The Farthest Man-Made Objects
planetary nebulae
Planetary Nebulae
planetary orbits
The Solar System | Planetary Orbits
Play Button
Partiview's User Interface
Pleiades star cluster
Seeing Uncertainty
Point of Interest
Your Initial Location | Starting from Home
changing
Flight Modes | Changing the Point of
Point Toggle Button
Partiview's User Interface
Polygon Toggle Button
Partiview's User Interface | Viewing the Solar System
Polysides Slider
Partiview's User Interface
Polysize Slider
Partiview's User Interface
proplyd
The Orion Nebula Model
Proxima Centauri
Proxima Centauri Is the
pulsars
Pulsars Are Spinning Neutron | Pulsars
quasar
Quasi-Stellar Objects (Quasars) | What Is a Quasar? | What Are Quasars?
discovery
Discovering Quasars
quasi-stellar objects
see quasar
radio light
Appendix: Electromagnetic Spectrum
radio sphere
Earth's Radio Sphere | The Radio Sphere
redshift
Quasi-Stellar Objects (Quasars) | The Cosmic Microwave Background | Appendix: Redshift and Distance
Reference Time Display
Partiview's User Interface
right ascension
Celestial Coordinates Resemble Earth's
Rotate Flight Mode
Flight Modes | Using the Keyboard to
Sagittarius dwarf spheroidal galaxy
Our Nearest Neighbor
see all command
Stellar Distances Are Determined
see command
Intrinsically Bright Stars Lie | Threshold the Stars
selecting data points
Flight Modes | Proxima Centauri Is the
Shapley, Harlow
Globular Clusters Are Mostly | Size of Our Star | Galaxy Image | Our Nearest Neighbor
slider
Alpha
Partiview's User Interface | The Band of the
Censize
Partiview's User Interface | Changing the Point of
Flight Path
Partiview's User Interface
FOV
Partiview's User Interface | What Do Other Data
Labelmin
Partiview's User Interface
Labelsize
Partiview's User Interface
Polysides
Partiview's User Interface
Polysize
Partiview's User Interface
range
linear
Partiview's User Interface
logarithmic
Partiview's User Interface
Slum
Partiview's User Interface | Exoplanetary Systems
Speed
Partiview's User Interface
Slider Menu
Partiview's User Interface
Slider Scale Button
Partiview's User Interface
Sloan Digital Sky Survey
Sloan Galaxy Survey
galaxies
Galaxy Surveys | Sloan Galaxy Survey
quasars
Quasar Surveys | Sloan Quasar Survey
stars
Sloan Stars
Slum Slider
Partiview's User Interface | Exoplanetary Systems
Small Magellanic Cloud
The Magellanic Clouds
spacecraft trajectories
The Farthest Man-Made Objects | Spacecraft Trajectories
speed of light
Appendix: Light-Travel Time and
Speed Slider
Partiview's User Interface
Speed Toggle Button
Partiview's User Interface
spiral galaxy
Galaxies | Data Variables
star
brightness
Stellar Brightness
color
Color Is Derived from
distance uncertainty
Distance Uncertainty
luminosity
Intrinsic Brightnesses
orbit
Stellar Orbits
parallax
Stellar Distances Are Determined | Appendix: Parallax and Distance
stars data group
AMNH Stars | AMNH Fixed Stars
stellar distance uncertainty
Distance Uncertainty | The Stellar Distance Uncertainty
stellar orbits
Stellar Orbits
supercluster
Galaxy Clusters and Superclusters | Clusters of Clusters
superclusters
Abell Galaxy Clusters and
supernova remnants
Supernova Remnants Are the | Supernova Remnants
T dwarf
Dwarf Catalog
textcment command
Changing the Label Color | Exoplanetary Systems
Texture Toggle Button
Partiview's User Interface
thresh command
Stellar Brightness | Seeing Only the Nearest | Galactic Census
Time Control Buttons
Partiview's User Interface
time controls
Back Button
Partiview's User Interface
Feed Button
Partiview's User Interface
Reference Time Display
Partiview's User Interface
Speed Slider
Partiview's User Interface
Speed Toggle Button
Partiview's User Interface
Time Control Buttons
Partiview's User Interface
Time Dial
Partiview's User Interface
Time Display
Partiview's User Interface
Trip Button
Partiview's User Interface
Time Dial
Partiview's User Interface
Time Display
Partiview's User Interface
toggle button
Box
Partiview's User Interface
Label
Partiview's User Interface
Point
Partiview's User Interface
Polygon
Partiview's User Interface | Viewing the Solar System
Speed
Partiview's User Interface
Texture
Partiview's User Interface
Translate Flight Mode
Flight Modes | Translate Flight Mode
trigonometric parallax
Appendix: Parallax and Distance
Trip Button
Partiview's User Interface
Tully density surface
Tully's Smoothed Density Surfaces
Tully galaxy catalog
Local Large-Scale Structure | Tully's Nearby Galaxies | Tully Galaxy Catalog
Two-degree Field Survey
2dF Galaxy Survey
two-micron all-sky survey
Two Micron (2MASS) All-Sky
ultraviolet light
Appendix: Electromagnetic Spectrum
Universe
age
The Distance Scale
baby picture
The WMAP Image
Big Bang
The Cosmic Microwave Background | The Cosmic Microwave Background | Microwave (WMAP) All-Sky Survey
expansion
The Distance Scale | Origin of the CMB | Appendix: Redshift and Distance
large-scale structure
Galaxies
look-back time
Appendix: Redshift and Distance
origin
The Cosmic Microwave Background | The Cosmic Microwave Background | Microwave (WMAP) All-Sky Survey
user interface
Partiview's User Interface
Virgo galaxy cluster
The Virgo Cluster
Virgo Supercluster
Galaxy Clusters and Superclusters
visible all-sky survey
The Band of the | Visible All-Sky Survey | Visible All-Sky Survey
visible light
Appendix: Electromagnetic Spectrum
void
Filaments and Voids
Voyager spacecraft
The Farthest Man-Made Objects
Wilkinson Microwave Anisotropy Probe
The Cosmic Microwave Background | Microwave (WMAP) All-Sky Survey
WMAP
see Wilkinson Microwave Anisotropy Probe
X-ray light
Appendix: Electromagnetic Spectrum


© 2002-2005 American Museum of Natural History
Last Modified: 2007-12-19 by Brian Abbott