RESEARCH BASE
Search 3,721 documents across 34 fields — every claim tier-rated by evidence
3,633 are the core, quality-scored corpus (34 lettered sections — see How We Work); the remaining 88 are cross-corpus synthesis documents (68 InterDocs, 12 Connections, 8 Theories) also indexed here.
12 results for "disk instability"
Q_3_08 — Planetary Formation and Protoplanetary Disks
Planets form within protoplanetary disks — rotationally supported structures of gas and dust orbiting newly formed stars, with typical masses of 0.1–10% of the stellar mass, radii of 10–1000 AU, and lifetimes of ~1–10 mi
ZH_1_04 — Nebra Sky Disk: Bronze Age Star Map Analysis
The Nebra sky disk (Himmelsscheibe von Nebra) is a bronze disk approximately 30 cm in diameter, decorated with gold-leaf appliqué representing the sun (or full moon), a crescent moon, stars (including a cluster interpret
ZF_1_11 — Rogue Waves, Freak Seas, and Extreme Ocean Events
Rogue waves (also called freak waves, abnormal waves, or episodic waves) are individual ocean surface waves that are at least twice the significant wave height (H_s — the average height of the highest one-third of waves
E_3_01 — Rise and Fall of Civilizations
Every complex civilization in recorded history has collapsed or been transformed beyond recognition. The Bronze Age collapse (~1177 BCE) destroyed the interconnected civilizations of the eastern Mediterranean within a si
Q_4_28 — Tachyon Physics: Theoretical Possibility
Tachyons are hypothetical particles that travel faster than the speed of light, first given rigorous theoretical treatment by Gerald Feinberg of Columbia University in 1967. The concept builds on a peculiar feature of sp
Q_2_11 — Stellar Populations, Metallicity, and Generations
Stars preserve the chemical fingerprint of the gas from which they formed, making them archaeological records of the universe's chemical history. Walter Baade (1944) recognized two distinct stellar populations: Populatio
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_09 — Binary Star Systems and X-Ray Sources
Most stars in the Milky Way exist in binary or multiple-star systems — estimates range from ~50% for solar-type stars to >70% for massive O/B stars. Binary star interactions drive some of the most energetic phenomena in
Q_2_01 — Black Holes, Singularities, and Information
Black holes are regions of spacetime where gravity is so extreme that nothing — not even light — can escape once it crosses the event horizon. Predicted by general relativity (Schwarzschild solution, 1916), regarded as m
Q_3_11 — Cosmic Reionization and First Stars
The Epoch of Reionization (EoR) refers to the period in cosmic history (~150 million to ~1 billion years after the Big Bang, redshifts z ≈ 15–6) when the first luminous sources — Population III (Pop III) stars, early gal
O_4_15 — Rogue Waves: Extreme Ocean Waves and the Physics of the Improbable
Rogue waves (also called freak waves, monster waves, or abnormal waves) — individual ocean waves that are exceptionally large relative to the surrounding sea state, typically defined as waves whose height exceeds 2.2 tim
O_3_18 — Rogue Waves: Extreme Ocean Dynamics and Nonlinear Wave Physics
Rogue waves (also called freak waves, killer waves, or extreme waves) are individual ocean waves whose height exceeds twice the significant wave height ($H > 2H_s$) of their surrounding sea state, appearing without warni
BROWSE BY SECTION — 3,721 documents across 34 fields