Asteroid
A rocky or metal body orbiting the Sun, smaller than a planet. Most are in the belt between Mars and Jupiter.
Sizes run from metres to hundreds of km.
source40 words you hear in space news, in plain English. Every one checked against an official science page (NASA, ESA, the IAU, NOAA or the Nobel committee); the source link is under each.
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A rocky or metal body orbiting the Sun, smaller than a planet. Most are in the belt between Mars and Jupiter.
Sizes run from metres to hundreds of km.
sourceThe average distance from Earth to the Sun, about 150 million km.
Used for distances inside the solar system.
sourceLights in the sky near the poles, made when charged particles from the Sun hit gases in Earth's upper atmosphere.
Called the northern or southern lights.
sourceThe scientific model in which the universe expanded from an extremely hot, dense state about 13.8 billion years ago.
It describes expansion everywhere, not an explosion at one point.
sourceA region where gravity is so strong that nothing, not even light, can escape once it crosses the edge (the event horizon).
The first image of one (M87*) was released in 2019.
sourceAn icy body that grows a glowing head and tails of gas and dust when it comes near the Sun.
Halley's Comet returns about every 76 years.
sourceOne of 88 areas of the sky defined by the IAU, usually named after the star pattern inside it.
The stars in one pattern are often very far apart from each other.
sourceThe faint glow of radiation left from the early universe, seen in every direction.
It dates from about 380,000 years after the Big Bang.
sourceThe unknown cause of the universe's expansion speeding up.
The discovery that the expansion is speeding up won the 2011 Nobel Prize in Physics.
sourceMatter that does not give off or reflect light but shows itself through gravity.
It is thought to make up most of the matter in the universe.
sourceOrbits the Sun, is round from its own gravity and is not a moon, but has not cleared its orbit of other objects.
Pluto has been one since 2006.
sourceWhen one body blocks the light of another. In a solar eclipse the Moon blocks the Sun; in a lunar eclipse Earth's shadow falls on the Moon.
Never look at a solar eclipse without proper eye protection.
sourceThe two days a year when the Sun is over the equator, so day and night are about equal everywhere.
Around 20 March and 22-23 September.
sourceThe boundary around a black hole beyond which nothing can return.
It is a boundary, not a solid surface.
sourceA planet that orbits a star other than the Sun.
More than 6,000 have been confirmed.
sourceA huge system of stars, gas, dust and dark matter held together by gravity.
We live in the Milky Way.
sourceThe pull between things with mass. It keeps the Moon around Earth and planets around the Sun.
On the Moon you would weigh about a sixth of your Earth weight.
sourceA ring of icy bodies beyond Neptune.
Pluto is one of its largest members.
sourceThe distance light travels in one year: about 9.46 trillion km. It measures distance, not time.
Light from the Sun takes about 8 minutes to reach us; from the nearest star, about 4.2 years.
sourceA measure of brightness in astronomy. Smaller numbers are brighter.
The Sun is about -27; the faintest stars seen by eye are about +6.
sourceThe streak of light when a small piece of space rock burns up in Earth's atmosphere. Also called a shooting star.
The rock in space is a meteoroid.
sourceA piece of space rock that survives the fall and lands on the ground.
Most come from asteroids.
sourceOur home galaxy, a barred spiral with hundreds of billions of stars.
On a dark night its disk looks like a faint band across the sky.
sourceA natural body that orbits a planet or another body.
Earth has one; Jupiter has over 100 and Saturn nearly 300.
sourceA cloud of gas and dust in space. Some are where stars are born; some are what dying stars leave behind.
The Orion Nebula can be seen with the naked eye from a dark place.
sourceThe collapsed core left after a massive star explodes: more mass than the Sun packed into a ball about 20 km across.
A sugar-cube-sized piece of it would weigh about a billion tonnes on Earth.
sourceThe curved path of one object around another, held by gravity.
The ISS orbits Earth about every 90 minutes.
sourceAbout 3.26 light-years: the distance at which a star's parallax angle (its tiny yearly wobble as Earth circles the Sun) is one arcsecond.
Astronomers use it for distances between stars and galaxies.
sourceA body that orbits the Sun, is round from its own gravity, and has cleared its orbit of other objects (IAU 2006 definition).
There are eight in our solar system.
sourceA spinning neutron star that sweeps beams of radiation past Earth, so it seems to pulse.
Some spin hundreds of times a second.
sourceA late stage of a star like the Sun, when it swells and cools at the surface.
The Sun will become one in about 5 billion years.
sourceThe stretching of light toward longer, redder wavelengths when its source moves away.
It showed that galaxies are moving apart.
sourceA sudden burst of energy and radiation from the Sun's surface.
Strong ones can cause radio blackouts on Earth.
sourceThe days when the Sun reaches its highest or lowest point in the sky at noon, giving the longest and shortest days.
Around 21 June and 21 December.
sourceLight spread out by wavelength. It reveals what a star is made of, how hot it is and how it moves.
A rainbow is a spectrum of sunlight.
sourceA huge ball of hot gas, mostly hydrogen and helium, that shines by nuclear fusion in its core.
The Sun is a star.
sourceThe powerful explosion of a star, which can briefly outshine a whole galaxy.
It spreads heavy elements into space.
sourceAn instrument that collects light (or other radiation) to see distant objects.
The James Webb Space Telescope observes mostly in infrared.
sourceThe small, dense, hot core left when a Sun-like star runs out of fuel.
The Sun will become one in billions of years.
sourceThe point in the sky directly above you.
The opposite point, below your feet, is the nadir.
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