# data[].attributes.body
displacement or difference in the apparent position of an objec

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a star showing a sudden large increase in brightness and then slowly returning to its original state over a few months.

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formed when a massive star runs out of fuel and collapses

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a distinct body of interstellar clouds. Originally, the term was used to describe any diffused astronomical object, including galaxies beyond the Milky Way.

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a continuous and distinctive band of stars that appears on plots of stellar color versus brightness.

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the great size or extent of something

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the distance light travels in one year

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any star having a relatively large radius for its mass and temperature

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a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. The word is derived from the Greek galaxias, literally "milky", a reference to the Milky Way

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The emission spectrum of a chemical element or chemical compound is the spectrum of frequencies of electromagnetic radiation emitted due to an atom or molecule making a transition from a high energy state to a lower energy state.

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in the frequency of sound, light, or other waves as the source and observer move toward

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a hypothetical form of matter thought to account for approximately 85% of the matter in the universe

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the reverse of a bright-line spectrum

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dark energy is an unknown form of energy that affects the universe on the largest scales

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an expanding, glowing shell of hot gas

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highly magnetized rotating compact star

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highly luminous objects in the early universe, thought to be powered by supermassive black holes

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the wavelength of the light is stretched, so the light is seen as 'shifted' towards the red part of the spectrum

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is a condition that is not limited to a specific set of values but can vary, without gaps, across a continuum.

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the science of the origin and development of the universe. Modern astronomy is dominated by the Big Bang theory, which brings together observational astronomy and particle physics.

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the emission or transmission of energy in the form of waves or particles through space or through a material medium.

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microwave background, in Big Bang cosmology, is electromagnetic radiation which is a remnant from an early stage of the universe

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an emission spectrum that consists of a continuum of wavelengths.

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form conspicuous configurations of objects or creatures in the sky.

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as viewed from a given latitude on Earth, that never sets below the horizon due to its apparent proximity to one of the celestial poles.

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a fixed luminous point in the night sky which is a large, remote incandescent body like the sun.

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The movement of a star across the sky

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massive stars

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powerful and luminous stellar explosion.

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stellar core remnant composed mostly of electron-degenerate matter

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shift in wavelengths of light toward the blue end of the spectrum as an object moves toward us in space.

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A black hole is a region of spacetime where gravity is so strong

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The Big Bang theory is the prevailing cosmological model explaining the existence of the observable universe from the earliest known periods through its subsequent large-scale evolution

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he appearance of real motion from a sequence of still images

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the magnitude of a celestial object as it is actually measured from the earth.

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Motion of a craft relative to the earth.

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Absolute magnitude is a measure of the luminosity of a celestial object, on an inverse logarithmic astronomical magnitude scale

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a spectrum of electromagnetic radiation transmitted through a substance, showing dark lines or bands due to absorption of specific wavelengths.

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dark areas that become apparent at the Sun's photosphere as a result of intense magnetic flux pushing up from further within the solar interior

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the central region where nuclear reactions consume hydrogen to form helium.

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an instrument that separates incoming light by its wavelength or frequency and records the resulting spectrum in some kind of multichannel detector, like a photographic plate

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a stream of charged particles released from the upper atmosphere of the Sun, called the corona

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A sudden eruption of magnetic energy on or near the surface of the sun, usually associated with sunspots and accompanied by bursts of electromagnetic radiation and particles.

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approximately 11-year cycle experienced by the Sun

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large eruptions of electromagnetic radiation from the Sun lasting from minutes to hours.

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The layer of a star that lies just outside the core, to which radiant energy is transferred from the core in the form of photons. In this layer, photons bounce off other particles, following fairly random paths until they enter the convection zone.

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large, bright, gaseous feature extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the solar corona.

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The positron or antielectron is the antiparticle or the antimatter counterpart of the electron.

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visible surface if the sun

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Nuclear fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles.

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A neutrino is a fermion that interacts only via the weak interaction and gravity

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the region around a planet dominated by the planet's magnetic field

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Granulation is the process of forming grains or granules from a powdery or solid substance

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a major disturbance of Earth's magnetosphere that occurs when there is a very efficient exchange of energy from the solar wind into the space environment surrounding Earth

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The act or process of discharging anything

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A coronal mass ejection is a significant release of plasma and accompanying magnetic field from the solar corona.

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the outer atmosphere of the Sun

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A region of turbulent plasma between a star's core and its visible photosphere at the surface, through which energy is transferred by convection

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the movement caused within a fluid by the tendency of hotter and therefore less dense material to rise, and colder, denser material to sink under the influence of gravity, which consequently results in transfer of heat.

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a reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star's outer atmosphere.

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a natural electrical phenomenon characterized by the appearance of streamers of reddish or greenish light in the sky, usually near the northern or southern magnetic pole.

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natural electrical phenomenon characterized by the appearance of streamers of reddish or greenish light in the sky, usually near the northern or southern magnetic pole.

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a natural electrical phenomenon characterized by the appearance of streamers of reddish or greenish light in the sky, usually near the northern or southern magnetic pole.

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actual or apparent motion of a body in a direction opposite to that of the (direct) motions of most members of the solar system or of other astronomical systems with a preferred direction of motion

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a process-oriented representation that emphasizes the influences, or flow, of information between modules.

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the system of planetary motions according to which the earth is at the center with the sun, moon, and planets revolving around it and each orbit except for the sun and moon is composed of a principal circle upon which moves a smaller circle carrying the plane

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the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

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period for a planet to orbit the Sun increases rapidly with the radius of its orbit.

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describe the orbits of planets around the Sun.

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each planet's orbit about the Sun is an ellipse

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Johannes Kepler was a German astronomer, mathematician, astrologer, natural philosopher and writer on music

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a property of matter by which it continues in its existing state of rest or uniform motion in a straight line, unless that state is changed by an external force.

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measured from or considered in relation to the center of the sun.

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the universal force of attraction acting between all matter.

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measured from or considered in relation to the center of the earth.

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an epicycle used to describe planetary orbits in the Ptolemaic system.

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deviation of a curve or orbit from circularity.

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a process-oriented representation that emphasizes the influences, or flow, of information between modules.

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model of the solar system centered on the Sun, with Earth and other planets moving around it, formulated by Nicolas Copernicus, and published in 1543