RESEARCH BASE
Search 3,717 documents across 34 fields — every claim tier-rated by evidence
19 results for "galaxy"
ZH_4_15 — Milky Way Mythology: Cultural Interpretations of the Galaxy Worldwide
The Milky Way — the luminous band of light stretching across the night sky, now understood as the disk of our home galaxy seen edge-on from within — has been one of humanity's most universally observed and mythologized c
Q_2_05 — Galaxy Formation, Structure, and Classification
Galaxies — gravitationally bound systems of stars, gas, dust, and dark matter — are the fundamental building blocks of the universe's large-scale structure. From Edwin Hubble's morphological classification (1926) to mode
Q_1_20 — Fractal Cosmology: Is the Universe Self-Similar Across Scales?
The observable universe organises matter into a staggering fractal-like web of galaxy filaments, walls, voids, and clusters — structures visible at scales from 1 Mpc (galaxy groups) to 600 Mpc (the Hercules-Corona Boreal
ZA_2_16 — Gravitational Lensing: Bending Light, Dark Matter Mapping, and Cosmic Magnification
Gravitational lensing — the deflection and focusing of light from distant sources by the gravitational field of intervening mass — is one of the most powerful predictions of Einstein's general relativity and has become a
ZH_5_12 — Citizen Astronomy: Variable Star Observers to Exoplanet Hunters
Astronomy is one of the very few sciences where non-professional observers — amateurs, hobbyists, and citizen scientists — continue to make significant, publishable contributions to research alongside professionals. This
Q_1_06 — Dark Matter and Dark Energy
Approximately 95% of the universe's total mass-energy content is invisible: ~27% dark matter and ~68% dark energy. Dark matter was first inferred by Fritz Zwicky (1933) from galaxy cluster dynamics and confirmed by Vera
Q_1_08 — Observable Universe and Cosmic Web
The observable universe has a diameter of ~93 billion light-years (comoving distance) and contains an estimated 2 trillion galaxies (Conselice et al. 2016), ~10²⁴ stars, and ~10⁸⁰ atoms. But its most striking feature is
Q_1_17 — Modified Gravity Theories (MOND, TeVeS, and Alternatives to Dark Matter)
Modified Newtonian Dynamics (MOND) is a hypothesis proposed by Mordehai Milgrom in 1983 that modifies Newton's second law at very low accelerations (below approximately 1.2 × 10⁻¹⁰ m/s²) to explain galaxy rotation curves
Q_4_05 — Modified Gravity Theories
Modified gravity theories propose that the observed discrepancies between luminous matter and gravitational dynamics — traditionally attributed to dark matter — instead result from a breakdown or modification of Newtonia
Q_4_24 — Modified Gravity Theories: MOND, TeVeS, and f(R) Gravity
Modified gravity theories propose that the observed discrepancies between luminous matter and dynamical mass in galaxies and galaxy clusters — conventionally attributed to dark matter — instead arise from a modification
Q_2_08 — Quasars and Active Galactic Nuclei
Quasars (quasi-stellar objects) and active galactic nuclei (AGN) are the most luminous persistent objects in the universe, powered by accretion of matter onto supermassive black holes (SMBHs, 10⁶–10¹⁰ M☉) at galaxy cente
Q_2_19 — Modified Gravity Theories: MOND, TeVeS & Alternatives to Dark Matter
Modified gravity theories propose that the observed discrepancies between predicted and measured gravitational effects in galaxies and galaxy clusters — conventionally attributed to dark matter — instead result from modi
Q_2_10 — Cosmic Voids and Large-Scale Structure
Cosmic voids are the most voluminous structures in the universe — vast, roughly spherical regions of space spanning 20–300 Mpc (65–1,000 million light-years) that contain far fewer galaxies than average. Together with fi
Q_3_04 — Gravitational Lensing: Bending Light and Mapping the Invisible Universe
Gravitational lensing — the bending of light by massive objects predicted by Einstein's general relativity — has become one of the most powerful observational tools in modern astrophysics. First confirmed during the 1919
ZB_5_20 — Citizen Science: Public Participation in Scientific Research
Citizen science — also termed community science, participatory science, or public participation in scientific research (PPSR) — involves non-professional volunteers in systematic data collection, analysis, or interpretat
G_4_12 — Citizen Science and Open-Source Research
Citizen science — the systematic involvement of non-professional volunteers in scientific research through data collection, classification, analysis, or distributed computation — has emerged as a powerful modern framewor
ZA_2_20 — Dark Matter & Dark Energy
Approximately 95% of the universe's total energy content consists of two components that have never been directly detected: dark matter (~26.4%) and dark energy (~68.7%), with ordinary baryonic matter comprising only ~4.
ZA_2_08 — Modified Gravity Theories: MOND, f(R), and Alternatives to Dark Matter
Modified gravity theories attempt to explain the "missing mass" problem — the discrepancy between observed gravitational effects and visible matter — without invoking dark matter particles. The most empirically successfu
ZA_3_11 — Cosmic Ray Physics and Ultra-High-Energy Particles
Cosmic rays — high-energy particles (primarily protons, alpha particles, and heavier atomic nuclei, with a small fraction of electrons and antimatter) that bombard Earth from space — were discovered by Victor Hess in 191
BROWSE BY SECTION — 3717 documents across 34 fields