Earth rotation

E21210

Earth rotation is the spinning of our planet on its axis, which produces the cycle of day and night and underlies the measurement of time.

AI illustration

How this image was made

AI-generated illustration of Earth rotation

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of Earth rotation (Earth rotation is the spinning of our planet on its axis, which produces the cycle of day and night and underlies the measurement of time.)

All labels observed (1)

Label Occurrences
Earth rotation canonical 3

How this entity was disambiguated

Statements (52)

Predicate Object
instanceOf astronomical phenomenon ⓘ
physical process ⓘ
rotational motion ⓘ
affects Coriolis effect ⓘ
Foucault pendulum precession ⓘ
ocean currents ⓘ
trade winds ⓘ
weather patterns ⓘ
angularVelocity about 7.2921159×10^-5 radians per second ⓘ
causes centrifugal acceleration at equator ⓘ
cycle of day and night ⓘ
equatorial bulge of Earth ⓘ
flattening at Earth poles ⓘ
defines Earth day ⓘ
sidereal day ⓘ
solar day ⓘ
equatorialLinearSpeed about 1670 kilometers per hour ⓘ
about 465 meters per second ⓘ
hasApproximatePeriod 23.934 hours ⓘ
86164 seconds ⓘ
hasAxis Earth axis ⓘ
hasType sidereal rotation ⓘ
solar rotation ⓘ
historicallyExplainedBy Copernican heliocentric model ⓘ
linked to: Copernican system
influences Earth’s gravity field ⓘ
Earth’s shape ⓘ
isDescribedBy angular velocity ⓘ
isFundamentalFor astronomical coordinate systems ⓘ
civil time ⓘ
time zones ⓘ
timekeeping systems ⓘ
isMeasuredBy Very Long Baseline Interferometry ⓘ
atomic time comparisons ⓘ
satellite laser ranging ⓘ
isObservedWith Foucault pendulum ⓘ
star trails in long-exposure photography ⓘ
isSlowingDown true ⓘ
occursOn Earth ⓘ
referenceFrame distant stars ⓘ
inertial frame ⓘ
requiresCorrection leap seconds ⓘ
rotationDirection counterclockwise as seen from north celestial pole ⓘ
prograde ⓘ
west-to-east ⓘ
siderealDayLength 23 hours 56 minutes 4 seconds ⓘ
slowdownCause gravitational interaction with Moon ⓘ
tidal friction ⓘ
slowdownRate about 1.7 milliseconds per century ⓘ
solarDayLength 24 hours (mean solar day) ⓘ
underlies definition of a day ⓘ
measurement of time ⓘ
wasDebatedIn Scientific Revolution ⓘ

How these facts were elicited

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Greenwich Mean Time → definedRelativeTo → Earth rotation ⓘ
Brian Luzum → fieldOfWork → Earth rotation ⓘ
Gérard Petit → fieldOfWork → Earth rotation ⓘ