RESEARCH BASE

Search 3,721 documents across 34 fields — every claim tier-rated by evidence

3,721 Documents 34 Sections 43,625 Citations 34,852 Keywords Indexed 4 Evidence Tiers

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.

5 results for "pebble accretion"

Q_3_08 Verified Cosmology & Physics

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

protoplanetary disk planet formation core accretion disk instability planetesimal pebble accretion
ZF_2_02 Verified Oceanography

ZF_2_02 — Coral Reef Systems: Ecology, Bleaching, and Paleoclimatology

This document focuses on the oceanographic dimensions of coral reef systems — reef geomorphology, their role as paleoclimate archives, and hydrodynamic interactions — complementing ZB_3_02 which covers the biological and

coral reef coral bleaching Great Barrier Reef symbiodinium zooxanthellae reef ecology
Q_2_08 Verified Cosmology & Physics

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

quasar active galactic nucleus AGN supermassive black hole accretion disk Seyfert galaxy
Q_2_09 Verified Cosmology & Physics

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

binary stars X-ray binary Roche lobe accretion disk mass transfer neutron star
Q_2_01 Verified Cosmology & Physics

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

black hole singularity event horizon Schwarzschild Kerr Hawking radiation