SpaceClass
Your space knowledge hub β interactive 3D exploration, comprehensive glossary, organization profiles, and guides to help you understand every data point on Celestia.
π NASA's EYES on the SOLAR SYSTEM
Explore the solar system in stunning 3D β fly between planets, follow spacecraft, and witness cosmic events in real-time. Powered by NASA/JPL.
Ask the AI Tutor
Confused about a space term? Type it below and get a simple explanation!
π Understanding Celestia's Data
Quick guides to help you understand what the numbers, charts, and indicators across Celestia actually mean.
Reading the Kp Index
AuraWatchThe Kp index (0-9) measures geomagnetic disturbance. Kp 0-2 means quiet conditions, Kp 3-4 is unsettled, Kp 5+ indicates a geomagnetic storm (G1-G5). Higher Kp = auroras visible at lower latitudes. Kp 7+ means auroras could be seen in mid-latitudes like London or New York.
Understanding NEO Hazard Data
SkyPulseNear-Earth Object data shows miss distance (how far it passes from Earth), diameter estimates (min/max), and relative velocity. "Potentially hazardous" means it passes within 0.05 AU (~7.5 million km) AND is larger than 140m. This doesn't mean impact is imminent β it's a monitoring classification.
Fire Confidence Levels
EarthWatchMODIS fire detections show brightness temperature (Kelvin) and confidence percentage. >90% = very likely fire; 75-89% = probable fire; 60-74% = possible fire; <60% = low confidence (could be volcanic activity, gas flares, or hot surfaces). Brighter = hotter fire.
Mars Sol vs Earth Date
MissionsA "sol" is a Martian solar day (24h 39m 35s). Sol 1 = the rover's first day on Mars. You can convert between sol and Earth date. Curiosity landed Aug 6, 2012 (Sol 0). Higher sol numbers = more recent photos. Some sols have no photos (rover was driving, sleeping, or in safe mode).
Solar Wind Speed & Density
AuraWatchNormal solar wind: ~400 km/s speed, ~5 protons/cmΒ³ density. During CME impacts: speed can exceed 800 km/s with density spikes to 20-50/cmΒ³. Higher speed + density = stronger geomagnetic effects. The Bz component of the magnetic field matters most β southward Bz enables aurora activity.
ISS Tracking Coordinates
SkyPulseThe ISS orbits at ~408 km altitude, traveling at 27,600 km/h. Latitude ranges from -51.6Β° to +51.6Β° (the orbital inclination). Longitude changes continuously. One full orbit takes ~90 minutes. The trail line shows recent orbital path β useful for predicting when it might pass over your location.
π Space Organizations
The agencies and companies pushing the boundaries of human space exploration.
NASA
National Aeronautics and Space AdministrationESA
European Space AgencyISRO
Indian Space Research OrganisationJAXA
Japan Aerospace Exploration AgencyRoscosmos
Roscosmos State CorporationCNSA
China National Space AdministrationSpaceX
Space Exploration Technologies Corp.CSA
Canadian Space AgencyKARI / KASA
Korea Aerospace Research Institute / Korea AeroSpace AdministrationNOAA SWPC
Space Weather Prediction Center (NOAA)π Space Dictionary
A comprehensive reference of space terminology β from fundamental concepts to the specific metrics shown across Celestia.
Light Year
FundamentalsThe distance light travels in one year β about 9.46 trillion km (5.88 trillion miles). Used to measure vast cosmic distances between stars and galaxies.
Astronomical Unit (AU)
FundamentalsThe average distance from Earth to the Sun β about 149.6 million km. Used to describe distances within our solar system.
Parsec
FundamentalsA unit of distance equal to about 3.26 light years. Derived from parallax measurements; commonly used in professional astronomy.
Redshift
FundamentalsWhen light from distant objects stretches to longer (redder) wavelengths, indicating they are moving away from us. Key evidence for the expanding universe.
Blueshift
FundamentalsWhen light from objects compresses to shorter (bluer) wavelengths, indicating they are moving toward us. The Andromeda galaxy is blueshifted.
Electromagnetic Spectrum
FundamentalsThe full range of electromagnetic radiation: radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, and gamma rays. Telescopes observe across multiple bands.
Doppler Effect
FundamentalsThe change in frequency of a wave relative to an observer moving relative to the source. Used to detect exoplanets and measure star velocities.
Escape Velocity
FundamentalsThe minimum speed needed to break free from a celestial body's gravitational pull without further propulsion. Earth's is about 11.2 km/s.
Gravity Assist
FundamentalsA technique where a spacecraft uses a planet's gravity to change speed and direction, saving fuel. Voyager missions famously used this.
Main Sequence Star
StarsA star in the longest phase of its life, fusing hydrogen into helium. Our Sun is a main sequence G-type star about halfway through its 10-billion-year lifespan.
Red Dwarf
StarsThe most common type of star in the universe β small, cool, and long-lived. Proxima Centauri (nearest star to our Sun) is a red dwarf.
White Dwarf
StarsThe dense remnant core of a low-to-medium mass star after it exhausts its fuel. About Earth-sized but with a mass comparable to the Sun.
Neutron Star
StarsAn incredibly dense remnant of a massive star's supernova. A teaspoon of neutron star material weighs about 6 billion tons.
Pulsar
StarsA rapidly rotating neutron star that emits beams of electromagnetic radiation. Can spin up to 716 times per second, detected as periodic radio pulses.
Magnetar
StarsA neutron star with an extraordinarily powerful magnetic field β a trillion times stronger than Earth's. The most magnetic objects in the known universe.
Black Hole
StarsA region of space where gravity is so strong that nothing, not even light, can escape. Formed from the collapse of massive stars or found at galaxy centers.
Supernova
StarsThe explosive death of a massive star, briefly outshining entire galaxies. Seeds space with heavy elements like iron, gold, and uranium.
Binary Star
StarsTwo stars that orbit around their common center of mass. Over half of all star systems are binaries or multiples.
Variable Star
StarsA star whose brightness changes over time, either due to internal pulsation or eclipsing by a companion. Cepheid variables are key distance markers.
Protostar
StarsA young star still gathering mass from its surrounding molecular cloud. Not yet hot enough for hydrogen fusion β the stage before becoming a main sequence star.
Terrestrial Planet
Solar SystemA rocky planet with a solid surface β Mercury, Venus, Earth, and Mars. Distinguished from gas and ice giants by composition.
Gas Giant
Solar SystemA large planet composed mainly of hydrogen and helium β Jupiter and Saturn. They lack a well-defined solid surface.
Ice Giant
Solar SystemA giant planet composed mainly of elements heavier than hydrogen/helium, like water, ammonia, and methane β Uranus and Neptune.
Dwarf Planet
Solar SystemA celestial body orbiting the Sun, massive enough for gravity to make it round, but not clearing its orbital neighborhood. Examples: Pluto, Ceres, Eris.
Asteroid Belt
Solar SystemA region between Mars and Jupiter containing millions of rocky objects β remnants of the early solar system that never formed into a planet.
Kuiper Belt
Solar SystemA region beyond Neptune extending from 30 to 55 AU, containing icy bodies including Pluto. Much larger than the asteroid belt.
Oort Cloud
Solar SystemA theoretical sphere of icy objects at the very edge of the Sun's influence, extending up to 100,000 AU. Source of long-period comets.
Lagrange Point
Solar SystemFive special positions where gravitational forces create stable "parking spots" for spacecraft. The James Webb Space Telescope orbits the L2 point.
Solar Wind
Solar SystemA stream of charged particles (plasma) released from the Sun's upper atmosphere at speeds of 400-800 km/s. Causes auroras on Earth.
Heliosphere
Solar SystemThe bubble of space dominated by the solar wind, extending far beyond Pluto. Voyager 1 crossed its boundary (heliopause) in 2012.
Magnetosphere
Solar SystemThe region around a planet dominated by its magnetic field. Earth's magnetosphere deflects solar wind and protects life from radiation.
Near-Earth Object (NEO)
Solar SystemAny asteroid or comet with an orbit that brings it within 1.3 AU of the Sun. NASA tracks over 30,000 NEOs for planetary defense.
Galaxy
CosmologyA vast system of stars, gas, dust, and dark matter bound together by gravity. The Milky Way contains an estimated 100-400 billion stars.
Nebula
CosmologyA giant cloud of gas and dust in space. Emission nebulae glow from ionized gas; reflection nebulae scatter starlight; dark nebulae block light behind them.
Dark Matter
CosmologyAn invisible substance making up ~27% of the universe. It doesn't emit or absorb light but exerts gravitational pull, holding galaxies together.
Dark Energy
CosmologyA mysterious force making up ~68% of the universe, driving its accelerating expansion. Discovered in 1998 through supernova observations.
Cosmic Microwave Background (CMB)
CosmologyAncient thermal radiation left over from the Big Bang, about 380,000 years after the universe formed. Fills all of space at 2.7 Kelvin.
Exoplanet
CosmologyA planet orbiting a star outside our solar system. Over 5,600 have been confirmed as of 2024, found via transit and radial velocity methods.
Habitable Zone
CosmologyThe region around a star where conditions could allow liquid water on a planet's surface. Also called the "Goldilocks zone" β not too hot, not too cold.
Gravitational Lensing
CosmologyThe bending of light by massive objects, predicted by Einstein's general relativity. Used to study dark matter and magnify distant galaxies.
Quasar
CosmologyAn extremely luminous active galactic nucleus powered by a supermassive black hole consuming matter. Some are visible billions of light years away.
Solar Flare
Space WeatherA sudden burst of electromagnetic radiation from the Sun's surface. Classified by X-ray intensity: A, B, C, M, X (strongest). Can disrupt radio communications.
Coronal Mass Ejection (CME)
Space WeatherA massive burst of solar wind and magnetic fields rising above the solar corona. When directed at Earth, can cause geomagnetic storms.
Geomagnetic Storm
Space WeatherA disturbance in Earth's magnetosphere caused by solar wind. Measured on the G1-G5 scale. Can affect power grids, GPS, and cause auroras at lower latitudes.
Kp Index
Space WeatherA 0-9 scale measuring geomagnetic activity. Kp β€ 2 is quiet; Kp 5+ indicates a geomagnetic storm. Used in Celestia's AuraWatch for aurora predictions.
Aurora (Northern/Southern Lights)
Space WeatherLuminous displays caused by charged particles from the Sun interacting with Earth's magnetic field and atmosphere. Visible near the poles, or globally during strong storms.
Sunspot
Space WeatherA dark region on the Sun's surface caused by magnetic activity. Sunspot count follows an 11-year solar cycle and correlates with space weather activity.
Solar Cycle
Space WeatherAn approximately 11-year cycle of solar magnetic activity. Solar maximum brings more sunspots, flares, and CMEs. We're currently in Solar Cycle 25 (peaked ~2024).
Radiation Belt
Space WeatherZones of energetic charged particles trapped by Earth's magnetic field. The Van Allen belts can pose hazards to satellites and astronauts.
Low Earth Orbit (LEO)
TechnologyOrbits between 160-2,000 km altitude. The ISS orbits at ~408 km. Most Earth observation and communication satellites operate in LEO.
Geostationary Orbit (GEO)
TechnologyAn orbit at ~35,786 km altitude where a satellite matches Earth's rotation, appearing stationary. Used for weather and communication satellites.
Delta-v
TechnologyThe change in velocity needed for orbital maneuvers. A key measure for mission planning β determines fuel requirements for reaching destinations.
Ion Thruster
TechnologyA propulsion system that creates thrust by accelerating ions using electricity. Very fuel-efficient but low thrust β ideal for deep space missions like Dawn.
Hohmann Transfer
TechnologyThe most fuel-efficient way to transfer between two circular orbits using two engine burns. Standard approach for missions to Mars and other planets.
Aerobraking
TechnologyUsing a planet's atmosphere to slow down a spacecraft and reduce its orbit, saving fuel. Used by Mars orbiters like Mars Reconnaissance Orbiter.
Space Debris
TechnologyNon-functional objects in orbit β defunct satellites, rocket stages, fragments. Over 36,000 objects larger than 10cm tracked; poses collision risks (Kessler syndrome).
Sol (Mars Day)
TechnologyA Martian day lasting about 24 hours 39 minutes. Mars rover missions count mission progress in sols. Curiosity has operated for over 4,000 sols.
MODIS
Earth ObservationModerate Resolution Imaging Spectroradiometer β a key instrument on NASA's Terra and Aqua satellites. Observes land, oceans, and atmosphere in 36 spectral bands.
FIRMS
Earth ObservationFire Information for Resource Management System β NASA's near-real-time fire detection system using MODIS and VIIRS satellite data. Powers Celestia's fire hotspot map.
EPIC Camera
Earth ObservationEarth Polychromatic Imaging Camera aboard DSCOVR at the L1 Lagrange point. Captures full-disc Earth images daily from 1.5 million km away.
DSCOVR
Earth ObservationDeep Space Climate Observatory β a NOAA satellite at the L1 point monitoring solar wind, space weather, and Earth's radiation budget.
VIIRS
Earth ObservationVisible Infrared Imaging Radiometer Suite β a sensor on Suomi NPP and NOAA-20 satellites providing high-res imagery for weather, fire detection, and ocean monitoring.
Remote Sensing
Earth ObservationAcquiring information about Earth from sensors on satellites or aircraft without physical contact. Includes optical, radar, and thermal imaging.