TubeTalk Pronunciation

How to pronounce “stellarity

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Pronunciation guide for stellarity

Learning goal
Practice the English pronunciation of stellarity with real speech in context.
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Definition summary
(astronomy) A parameter (between 0.0 and 1.0), generated by a neural network, that seeks to characterize how stellar an observed astronomical object is.

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A Deep Dive Into “stellarity

Meaning

  • [Noun]
  • (astronomy) A parameter (between 0.0 and 1.0), generated by a neural network, that seeks to characterize how stellar an observed astronomical object is.

Practice Nearby Words

variable star, luminosity function, variable, statefinder, spectral type, apparent brightness, luminosity, quasi-stellar object, scalar field, photometry, initial mass function, apparent magnitude, bolometric magnitude, antistar, visual magnitude, star cluster, linestrength, stilb, starburst, state variable, isoscalar, stellation, planck star, magnitude, boson star, balnicity, statevector, space velocity, radiometric magnitude, scintillation, velocity dispersion, absolute magnitude, compact star, parameter, helium variable, signal-to-noise ratio, mode, spin polarization, sterino, quasistar, occupation number, bandstrength, perturbation, spectral class, quasi-stellar radio-source, metallicity, constant, strange star, modulus, quasi-star, true strain, gravastar, strouhal number, spatiality, rayleigh, renormalon, strangeness, minimum, protostar, electron density, magicity, przybylski's star, temperature, classicality, exotic star, symmetron, isospin, standing stock, standard deviation, starburst galaxy, yrast, space motion, virialization, starlight, quasi-stellar radio source, gamnitude, absolute space, spectroastrometry, stark effect, exceptional space, fine structure constant, fine-structure constant, bolometric correction, sommerfeld parameter, hyperentropy, hapke parameter, metastability, steradiancy, stellar wind, runaway star, responsivity, snark, dark star, polarization vector, signal-to-noise, signal strength, space quantization, active galactic nucleus, quasi-stellar radiosource, nongaussianity

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