Celestial Atlas · LearnOpen the 3D atlas ▸

Celestial Atlas › Learn › Glossary

Astronomy glossary

69 terms used in Celestial Atlas, defined in one or two sentences each. Terms link to the pages where they appear in context.

Albedo
The fraction of incoming sunlight a surface reflects. Earth's is about 0.30, Venus's about 0.76. It sets a planet's equilibrium temperature.
Altitude and azimuth
A position in the sky measured from your horizon: altitude is the angle above the horizon (0° to 90°), azimuth the compass bearing (N 0°, E 90°, S 180°, W 270°). Used in the Sky view.
Annular eclipse
A solar eclipse in which the Moon is too far from Earth to cover the Sun completely, leaving a bright ring (“ring of fire”). See eclipses.
Aphelion and perihelion
The farthest and nearest points of a body's orbit around the Sun. Earth's perihelion is about 147.1 million km in early January; its aphelion about 152.1 million km in early July.
Apogee and perigee
The farthest and nearest points of the Moon's orbit around Earth (about 405,500 km and 363,300 km).
Arcsecond
1/3,600 of a degree. The Moon's disc is about 1,800 arcseconds wide; the accuracy of the atlas's planet positions is a few arcseconds.
Asymptotic giant branch (AGB)
The final giant phase of a Sun-like star, after helium burning, when it swells again and sheds its outer layers. See the Sun's life.
Astronomical unit (AU)
The average distance between Earth and the Sun, about 149.6 million km; light needs 499 seconds to cross it.
Barred spiral galaxy
A spiral galaxy with a straight bar of stars across its centre. The Milky Way, NGC 1300 and the Large Magellanic Cloud have bars.
Black dwarf
The hypothetical end state of a white dwarf after it has cooled completely, expected to take far longer than the age of the Universe.
Bloom
A graphic effect that adds a soft glow around very bright objects. It can be switched off in Options.
Bulge (galactic)
The central, roughly spheroidal swelling of old stars in a spiral galaxy; the Milky Way's is boxy or peanut-shaped.
Celestial sphere
The imaginary sphere on which stars appear to lie, centred on the observer, used to describe directions in the sky.
Chandrasekhar dynamical friction
The gravitational drag a massive body feels as it moves through a sea of lighter particles such as a dark-matter halo, causing galaxies on close orbits to lose energy and merge. Used in the collision simulation.
Civil, nautical and astronomical twilight
Stages of dusk and dawn when the Sun is 0–6°, 6–12° and 12–18° below the horizon. See Sky view.
Climatology
The statistical average of weather for a place, date and time of day over many years. Shown instead of a forecast when none exists.
Conjunction
When two bodies appear at the same ecliptic longitude as seen from Earth; a planet is in conjunction with the Sun when it is in line with it.
Corona
The Sun's outer atmosphere, visible as a white halo only during a total solar eclipse.
Cosmic microwave background (CMB)
The faint microwave glow left over from the early Universe. Its slight dipole reveals our motion: the Sun moves at about 370 km/s relative to it.
Dark matter
Invisible matter detected only through its gravity, which makes up most of every galaxy's mass. In the collision simulation it is the halo that does the pulling.
Dwarf spheroidal galaxy
A faint, round or elliptical galaxy with few stars and little gas, such as Draco, Sculptor and Fornax around the Milky Way.
Ecliptic
The plane of Earth's orbit around the Sun, and the apparent yearly path of the Sun among the stars. Planets lie close to it.
Elliptical galaxy
A smooth, roughly ellipsoidal galaxy of old stars with little gas and no spiral arms; the likely product of a major merger.
Elongation
The angle between a planet and the Sun as seen from Earth. Mercury's maximum is about 28°, Venus's about 47°.
ERA5
A global hourly reanalysis of the weather since 1940 produced by ECMWF/Copernicus, used for historical weather in the atlas.
Equilibrium temperature
The temperature a planet would have if it balanced absorbed sunlight against emitted heat, ignoring any greenhouse effect: T = 278.5 K × (1−A)¼ L¼ / √a, with albedo A, luminosity L in solar units and distance a in AU.
Equinox and solstice
Moments when the Sun is over the equator (equinox, near 20 March and 22–23 September) or at its farthest north or south (solstice, near 21 June and 21 December).
Gaia
The European Space Agency's astrometry mission (launched 2013) that measures the positions, distances and motions of over a billion stars. See Gaia stars.
Galactic year
One orbit of the Sun around the Galactic Centre, about 223 million years.
Gould Belt
A tilted ring of young stars and star-forming clouds about 700 pc across around the Sun, including Orion and Scorpius–Centaurus.
Great Attractor
A massive concentration of galaxies in the Norma region, about 220 million light-years away, toward which our local supercluster flows.
Habitable zone
The range of distances from a star where a rocky planet could keep liquid water on its surface. Today 0.95–1.68 AU for the Sun by the simple limits used in the atlas.
Helium flash
The sudden ignition of helium fusion in the degenerate core of a red giant, at the tip of the red-giant branch.
Hubble Space Telescope
NASA/ESA's orbiting observatory, launched 1990, source of the photographs of M51, M104, NGC 1300, NGC 4414 and the Antennae used in the atlas.
Julian day
A continuous count of days used by astronomers; the atlas converts every date to a Julian day (and UTC) for its calculations.
Kiloparsec (kpc)
1,000 parsecs, about 3,262 light-years. The Sun is 8.18 kpc from the Galactic Centre.
Laniakea
The supercluster of about 100,000 galaxies, 520 million light-years across, that contains the Milky Way. See Laniakea.
Libration
The apparent wobble of the Moon that lets us see about 59% of its surface over time.
Light-year
The distance light travels in a year: 9.46 trillion km (63,241 AU).
Limiting magnitude
The faintest star visible under given conditions; about 6.5 in a dark sky.
Local Bubble
A cavity about 100 parsecs wide of hot, thin gas around the Sun, carved by supernovae.
Local Group
The gravitationally bound group of about 80 galaxies including the Milky Way, Andromeda and Triangulum.
Magnitude
A logarithmic brightness scale in which smaller numbers are brighter: the Sun −26.7, the full Moon −12.7, Venus up to −4.9, the faintest naked-eye stars about +6.5.
Main sequence
The long phase in a star's life when it fuses hydrogen to helium in its core. The Sun has been on it for 4.57 billion years and will remain for about 5.4 billion more.
Milkomeda
A nickname for the single elliptical galaxy that the Milky Way and Andromeda may form. See the collision.
Moist greenhouse
A climate state in which a warming planet's stratosphere fills with water vapour, which escapes to space; the first step in losing oceans. It begins at roughly 1.1 times Earth's present sunlight.
Node (lunar)
One of the two points where the Moon's orbit crosses the ecliptic. Eclipses occur when New or Full Moon happens near a node.
Obscuration
The fraction of the Sun's disc area covered by the Moon during a solar eclipse.
Parallax
The apparent shift of a nearby star against distant ones as Earth orbits the Sun; a star with 1 arcsecond parallax is 1 parsec away.
Parsec (pc)
3.26 light-years; the distance at which one AU subtends one arcsecond.
Peculiar velocity
A body's motion relative to its local rest frame, such as the Sun's 18–20 km/s relative to nearby stars or a galaxy's flow relative to the Hubble expansion.
Penumbra
The partial shadow where only part of the Sun is hidden. In a lunar eclipse, the faint outer part of Earth's shadow.
Planetary nebula
A shell of gas ejected by a dying Sun-like star and lit by its hot core; unrelated to planets.
Prograde and retrograde
Moving or spinning in the same sense as an orbit (prograde) or the opposite sense (retrograde).
Proper motion
A star's apparent change of position on the sky over time, in arcseconds per year. Sirius moves 1.33″ per year.
Red giant
A star that has used up the hydrogen in its core and swollen to tens or hundreds of times its former radius, with a cool, red surface.
Saros
An eclipse cycle of 6,585.3 days (18 years 11 days 8 hours) after which Sun, Moon and nodes return to almost the same geometry, so similar eclipses recur.
Sidereal day
The time Earth takes to rotate once relative to the stars: 23 h 56 min 4 s.
Sidereal and synodic month
The Moon's orbit relative to the stars (27.32 days) and its cycle of phases (29.53 days).
Spiral arm
A curved band of stars, gas and dust in a spiral galaxy. The Milky Way has four main arms; the Sun lies in the Orion Spur between two of them.
Supercluster
A vast region containing many galaxy groups and clusters, tens to hundreds of millions of light-years across.
Supermassive black hole
A black hole of millions to billions of solar masses at the centre of a galaxy. The Milky Way's, Sagittarius A*, has about 4 million.
Synodic period
The time between successive similar alignments, such as the same Moon phase or a planet's return to opposition.
Tidal tail
A long stream of stars pulled out of a galaxy by the gravity of a close neighbour during an encounter.
Totality
The phase of a total solar eclipse when the Sun is completely covered, lasting up to about 7½ minutes.
True scale
A display mode in which bodies and distances are drawn at their real relative sizes (1 scene unit = 1,000 km in the atlas).
Umbra
The darkest part of a shadow, where the light source is fully hidden. Observers in the Moon's umbra see a total solar eclipse.
White dwarf
The dense, Earth-sized remnant of a Sun-like star that has shed its outer layers; the Sun will become one of about 0.54 solar masses.
ΔT (delta T)
The difference between uniform time and time based on Earth's irregular rotation; it limits how precisely eclipses far in the past or future can be timed.