Cosmik

Learn space: every question, answered with live data

Every space explainer, definition, live-data page and tracker on Cosmik, indexed in one place — so any answer is at most two clicks away.

This is the Cosmik encyclopedia: a single index of everything we explain about space, from what a star is to where Artemis II is right now. Every explainer, glossary definition, live-data page and tracker below is at most two clicks away — and the answers are backed by real-time positions and counts, not static text.

Questions & explainers

Plain-language answers to the big questions, each linking straight to the live 3D view.

Glossary

Every space term in one-line definitions. See the full space glossary, or jump straight to a term.

Orbits & orbital mechanics

  • LEO (low Earth orbit)Low Earth orbit (LEO) is the region of space from about 160 to 2,000 km above Earth's surface, where satellites circle the planet in roughly 90 minutes.
  • MEO (medium Earth orbit)Medium Earth orbit (MEO) is the band from about 2,000 km up to the geostationary altitude of 35,786 km, best known as the home of navigation satellites.
  • GEO (geostationary Earth orbit)Geostationary orbit (GEO) is the circular orbit 35,786 km above the equator where a satellite's period exactly matches Earth's rotation, so it appears fixed over one spot.
  • HEO (highly elliptical orbit)A highly elliptical orbit (HEO) is a stretched, egg-shaped orbit with a low perigee and a very high apogee, letting a satellite linger for hours over one hemisphere.
  • Sun-synchronous orbit (SSO)A sun-synchronous orbit (SSO) is a near-polar low Earth orbit tuned so the satellite passes over every location at the same local solar time on each visit.
  • Geostationary satelliteA geostationary satellite orbits 35,786 km above the equator in step with Earth's rotation, so from the ground it appears to hang motionless in the sky.
  • ApogeeApogee is the point in an orbit around Earth where the satellite is farthest from the planet.
  • PerigeePerigee is the point in an orbit around Earth where the satellite is closest to the planet.
  • Orbital inclinationOrbital inclination is the angle between a satellite's orbital plane and Earth's equator, measured in degrees.
  • RAAN & the ascending nodeThe ascending node is where a satellite crosses the equator heading north; RAAN (right ascension of the ascending node) is the angle that fixes that crossing point in space.
  • Lagrange pointA Lagrange point is one of five positions in a two-body system, such as the Sun and Earth, where gravity and orbital motion balance so a spacecraft can hold station with little fuel.
  • Orbital periodThe orbital period is the time a satellite takes to complete one full orbit, set almost entirely by its altitude.
  • Ground trackA ground track is the path traced on Earth's surface directly beneath a satellite as it orbits.
  • Satellite constellationA satellite constellation is a group of satellites working together as one system to give continuous or global coverage that a single satellite cannot.

Launch & reentry

  • Delta-v (Δv)Delta-v (Δv) is the change in velocity a spacecraft must produce to perform a manoeuvre — launching, changing orbit or landing — and it is the basic currency of orbital mechanics.
  • Max-QMax-Q is the moment during a rocket launch when aerodynamic pressure on the vehicle is at its greatest, usually about a minute after liftoff.
  • Atmospheric reentryAtmospheric reentry is the return of a spacecraft or piece of debris into Earth's atmosphere, where friction and compression heat it to thousands of degrees.

Tracking & data

  • GNSS (global navigation satellite system)GNSS is the umbrella term for the satellite constellations that provide positioning, navigation and timing — GPS, Galileo, GLONASS and BeiDou.
  • Ground sample distance (GSD)Ground sample distance (GSD) is the real-world distance on the ground covered by one pixel of a satellite or aerial image — the core measure of spatial resolution.
  • TLE (two-line element set)A TLE (two-line element set) is a compact, standardized text format that encodes a satellite's orbit at a specific moment in two 69-character lines.
  • SGP4SGP4 is the standard mathematical model that turns a satellite's TLE into a predicted position and velocity at any given time.
  • Kessler syndromeKessler syndrome is a scenario in which collisions between orbiting objects create debris that triggers more collisions, cascading until parts of low Earth orbit become hazardous to use.
  • ConjunctionIn satellite tracking, a conjunction is a close approach between two orbiting objects — a predicted near-miss operators watch in case a collision-avoidance manoeuvre is needed.

Space weather

  • Kp indexThe Kp index is a 0–9 scale of global geomagnetic activity over three-hour periods, and it is the number aurora watchers check to judge tonight's odds.
  • Geomagnetic stormA geomagnetic storm is a temporary disturbance of Earth's magnetic field driven by bursts of solar wind and coronal mass ejections from the Sun.

Sky & observing

  • AzimuthAzimuth is the compass direction to an object in the sky, measured in degrees clockwise from true north — 0° is north, 90° east, 180° south, 270° west.
  • Twilight (civil, nautical, astronomical)Twilight is the period before sunrise and after sunset when the sky is partly lit by the Sun below the horizon, split into civil, nautical and astronomical stages.
  • Aphelion (& perihelion)Aphelion is the point in a body's orbit around the Sun where it is farthest from the Sun; perihelion is the closest point.

Live data, by question

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