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πŸ“Š Understanding Celestia's Data

Interpretability

Quick guides to help you understand what the numbers, charts, and indicators across Celestia actually mean.

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Reading the Kp Index

AuraWatch

The 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.

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Understanding NEO Hazard Data

SkyPulse

Near-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.

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Fire Confidence Levels

EarthWatch

MODIS 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.

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Mars Sol vs Earth Date

Missions

A "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).

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Solar Wind Speed & Density

AuraWatch

Normal 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.

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ISS Tracking Coordinates

SkyPulse

The 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.

πŸš€ Space Organizations

10 Agencies

The agencies and companies pushing the boundaries of human space exploration.

NASA

National Aeronautics and Space Administration
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United StatesEst. 1958Washington, D.C.

ESA

European Space Agency
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Europe (22 member states)Est. 1975Paris, France

ISRO

Indian Space Research Organisation
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IndiaEst. 1969Bengaluru, India

JAXA

Japan Aerospace Exploration Agency
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JapanEst. 2003Chōfu, Tokyo

Roscosmos

Roscosmos State Corporation
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RussiaEst. 1992Moscow, Russia

CNSA

China National Space Administration
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ChinaEst. 1993Beijing, China

SpaceX

Space Exploration Technologies Corp.
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United States (Private)Est. 2002Hawthorne, California

CSA

Canadian Space Agency
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CanadaEst. 1989Saint-Hubert, Quebec

KARI / KASA

Korea Aerospace Research Institute / Korea AeroSpace Administration
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South KoreaEst. 1989Daejeon, South Korea

NOAA SWPC

Space Weather Prediction Center (NOAA)
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United StatesEst. 1965Boulder, Colorado

πŸ“– Space Dictionary

63 Terms

A comprehensive reference of space terminology β€” from fundamental concepts to the specific metrics shown across Celestia.

Showing 63 of 63 terms

Light Year

Fundamentals

The 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)

Fundamentals

The average distance from Earth to the Sun β€” about 149.6 million km. Used to describe distances within our solar system.

Parsec

Fundamentals

A unit of distance equal to about 3.26 light years. Derived from parallax measurements; commonly used in professional astronomy.

Redshift

Fundamentals

When light from distant objects stretches to longer (redder) wavelengths, indicating they are moving away from us. Key evidence for the expanding universe.

Blueshift

Fundamentals

When light from objects compresses to shorter (bluer) wavelengths, indicating they are moving toward us. The Andromeda galaxy is blueshifted.

Electromagnetic Spectrum

Fundamentals

The full range of electromagnetic radiation: radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, and gamma rays. Telescopes observe across multiple bands.

Doppler Effect

Fundamentals

The 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

Fundamentals

The 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

Fundamentals

A technique where a spacecraft uses a planet's gravity to change speed and direction, saving fuel. Voyager missions famously used this.

Main Sequence Star

Stars

A 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

Stars

The 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

Stars

The 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

Stars

An incredibly dense remnant of a massive star's supernova. A teaspoon of neutron star material weighs about 6 billion tons.

Pulsar

Stars

A rapidly rotating neutron star that emits beams of electromagnetic radiation. Can spin up to 716 times per second, detected as periodic radio pulses.

Magnetar

Stars

A 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

Stars

A 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

Stars

The explosive death of a massive star, briefly outshining entire galaxies. Seeds space with heavy elements like iron, gold, and uranium.

Binary Star

Stars

Two stars that orbit around their common center of mass. Over half of all star systems are binaries or multiples.

Variable Star

Stars

A star whose brightness changes over time, either due to internal pulsation or eclipsing by a companion. Cepheid variables are key distance markers.

Protostar

Stars

A 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 System

A rocky planet with a solid surface β€” Mercury, Venus, Earth, and Mars. Distinguished from gas and ice giants by composition.

Gas Giant

Solar System

A large planet composed mainly of hydrogen and helium β€” Jupiter and Saturn. They lack a well-defined solid surface.

Ice Giant

Solar System

A giant planet composed mainly of elements heavier than hydrogen/helium, like water, ammonia, and methane β€” Uranus and Neptune.

Dwarf Planet

Solar System

A 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 System

A 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 System

A region beyond Neptune extending from 30 to 55 AU, containing icy bodies including Pluto. Much larger than the asteroid belt.

Oort Cloud

Solar System

A 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 System

Five special positions where gravitational forces create stable "parking spots" for spacecraft. The James Webb Space Telescope orbits the L2 point.

Solar Wind

Solar System

A 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 System

The bubble of space dominated by the solar wind, extending far beyond Pluto. Voyager 1 crossed its boundary (heliopause) in 2012.

Magnetosphere

Solar System

The 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 System

Any 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

Cosmology

A vast system of stars, gas, dust, and dark matter bound together by gravity. The Milky Way contains an estimated 100-400 billion stars.

Nebula

Cosmology

A 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

Cosmology

An invisible substance making up ~27% of the universe. It doesn't emit or absorb light but exerts gravitational pull, holding galaxies together.

Dark Energy

Cosmology

A mysterious force making up ~68% of the universe, driving its accelerating expansion. Discovered in 1998 through supernova observations.

Cosmic Microwave Background (CMB)

Cosmology

Ancient 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

Cosmology

A 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

Cosmology

The 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

Cosmology

The bending of light by massive objects, predicted by Einstein's general relativity. Used to study dark matter and magnify distant galaxies.

Quasar

Cosmology

An extremely luminous active galactic nucleus powered by a supermassive black hole consuming matter. Some are visible billions of light years away.

Solar Flare

Space Weather

A 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 Weather

A massive burst of solar wind and magnetic fields rising above the solar corona. When directed at Earth, can cause geomagnetic storms.

Geomagnetic Storm

Space Weather

A 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 Weather

A 0-9 scale measuring geomagnetic activity. Kp ≀ 2 is quiet; Kp 5+ indicates a geomagnetic storm. Used in Celestia's AuraWatch for aurora predictions.

Aurora (Northern/Southern Lights)

Space Weather

Luminous 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 Weather

A 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 Weather

An 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 Weather

Zones 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)

Technology

Orbits between 160-2,000 km altitude. The ISS orbits at ~408 km. Most Earth observation and communication satellites operate in LEO.

Geostationary Orbit (GEO)

Technology

An orbit at ~35,786 km altitude where a satellite matches Earth's rotation, appearing stationary. Used for weather and communication satellites.

Delta-v

Technology

The change in velocity needed for orbital maneuvers. A key measure for mission planning β€” determines fuel requirements for reaching destinations.

Ion Thruster

Technology

A 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

Technology

The most fuel-efficient way to transfer between two circular orbits using two engine burns. Standard approach for missions to Mars and other planets.

Aerobraking

Technology

Using 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

Technology

Non-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)

Technology

A 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 Observation

Moderate 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 Observation

Fire 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 Observation

Earth Polychromatic Imaging Camera aboard DSCOVR at the L1 Lagrange point. Captures full-disc Earth images daily from 1.5 million km away.

DSCOVR

Earth Observation

Deep Space Climate Observatory β€” a NOAA satellite at the L1 point monitoring solar wind, space weather, and Earth's radiation budget.

VIIRS

Earth Observation

Visible 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 Observation

Acquiring information about Earth from sensors on satellites or aircraft without physical contact. Includes optical, radar, and thermal imaging.