Cosmic void

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feminine noun (astronomy / cosmology / rare)

Definition

A neologistic astronomical term used theoretically or hypothetically to describe a state or cosmic space characterized by the complete absence of galaxies; a vast region in the deep universe devoid of organized stellar structures or galactic systems.

Bilingual Equivalents

  • Cosmic void
  • Agalaxia

Grammatical & Source Details

Inflection Type Feminine noun with regular structural plural and case inflections.
Formation Neologism created by adding the private Greek prefix 'a-' to the core noun 'galaxie'.
Spelling / Pronunciation [a.ɡa.lak.ˈsi.e]
Source Lexicon of Theoretical Astrophysics and Cosmological Scale Metrics

Contextual Usage Examples

RO: Astrofizicienii au analizat radiația de fond dintr-o regiune de agalaxie profundă pentru a înțelege expansiunea universului.

EN: Astrophysicists analyzed background radiation from a deep cosmic void region to understand the expansion of the universe.

RO: Această agalaxie ipotetică ar putea reprezenta un stadiu timpuriu în evoluția structurală a macrocosmosului.

EN: This hypothetical anagalaxy could represent an early stage in the structural evolution of the macrocosm.

RO: Telescopul spațial a transmis imagini dintr-un sector marcat de agalaxie, unde materia întunecată predomină.

EN: The space telescope transmitted images from a sector marked by emptiness, where dark matter predominates.

Idioms & Phrases

Zonă de agalaxie / Galactic void zone

RO: Sector uriaș din spațiul cosmic în care densitatea galaxiilor este extrem de scăzută sau nulă conform observațiilor.

EN: A massive sector in outer space where the density of galaxies is extremely low or non-existent according to observations.

Agalaxie absolută / Absolute cosmic emptiness

RO: Model teoretic ce descrie un spațiu complet izolat, lipsit de orice formă de materie barionică organizată.

EN: A theoretical model describing a completely isolated space, devoid of any form of organized baryonic matter.

Efect de agalaxie / Void effect

RO: Fenomen cosmologic de lentilă gravitațională slabă observat la marginea marilor spații goale din univers.

EN: A cosmological phenomenon of weak gravitational lensing observed at the edges of large empty spaces in the universe.

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