The Living Archive.

“The science and art of planning, designing, and constructing buildings or other physical structures in a “functional” and “aesthetic” manner.”

“A catastrophic explosive event of a massive “star” marking the end of its life cycle, resulting in the release of immense energy and the formation of heavy chemical elements in the universe.”

“Small celestial bodies composed of rock and metal that orbit the Sun, primarily located within the “asteroid belt” between Mars and Jupiter.”

“An anatomical term referring to the “front” or belly side of an organism. It is used to describe the position of body structures located toward the anterior surface in humans or the underside in quadrupeds.”

“The act of “reaching” a point, touching, or holding an object physically or metaphorically. It can also be interpreted as holding something.”

“A facial expression characterized by a “radiant”, cheerful, and enthusiastic appearance that reflects a positive mood.”

“The actual state of affairs or objective facts occurring in reality. This term refers to “reality” which is often contrasted with hopes or fantasies.”

“Moral messages, guidance, or life advice given by elders or wise figures to provide behavioral “enlightenment” to others.”

“The point in the orbit of a planet, comet, or other celestial body that is nearest to the Sun. This phenomenon occurs due to the elliptical nature of orbital paths, where the object reaches its maximum orbital velocity while passing through this position.”

“The point in the orbit of a celestial body, such as a planet or comet, at which it is at its “farthest” distance from the Sun.”

“An astronomical coordinate system indicating the position of a celestial body on the celestial sphere, measured eastward from the “vernal equinox” along the celestial equator, typically expressed in units of hours, minutes, and seconds.”

“The angular distance of a celestial body measured north or south from the “celestial equator” along a declination circle. It is expressed in degrees, minutes, and seconds of arc.”

“The vertical distance or “angle” of a celestial body above the observer's horizon measured in degrees. This term refers to the relative position of astronomical objects to the local “horizon” line.”

“The orbital plane of the Earth around the Sun that forms an imaginary circle across the celestial sphere over one year. This path represents the apparent path of the Sun's center as viewed from Earth and serves as the primary reference for celestial coordinates.”

“A closed plane curve that is symmetrical and resembles an elongated circle, geometrically defined as the set of points where the sum of distances from two fixed points or “foci” remains constant.”

“The angular distance between two celestial bodies as seen from Earth, typically used to describe the position of a “planet” relative to the Sun.”

“The outermost layer of the sun or a star that emits energy as “electromagnetic radiation” in the visible light spectrum, making it visually observable.”

“The outermost layer of the Sun atmosphere resembling a white light “crown” and can only be visually observed during a total solar eclipse.”

“Pertaining to or originating from beyond the atmosphere or physical boundaries of planet Earth. This term refers to any phenomena, celestial bodies, or hypothetical biological entities existing in outer space or other worlds outside the terrestrial system.”

“A highly magnetized and rapidly rotating neutron star that emits beams of electromagnetic radiation from its magnetic poles. This dense celestial object is observed as regular pulses of radiation as its emission beam points toward Earth at fixed intervals.”

“An extremely remote and highly luminous active galactic nucleus, powered by an accretion disk surrounding a supermassive black hole. This object emits immense amounts of electromagnetic energy, appearing star-like through telescopes, and serves as one of the most brilliant entities in the universe.”

“The apparent displacement or difference in the position of an object viewed along two different lines of sight. This phenomenon is commonly used in “astronomy” to measure the distance of celestial bodies.”

“The total amount of energy emitted by an astronomical object such as a star per unit of time. It is typically measured in “watts” or expressed in multiples of the Sun's luminosity.”

“A quantitative measure indicating the degree of brightness or light intensity of an astronomical object on a logarithmic scale. A lower numerical value signifies a brighter luminosity. This term refers to the physical magnitude that classifies celestial bodies based on the received radiative energy.”