Cosmic construction

From matter to the Universe
Gas and dust → planets and stars → stellar systems → galaxies → large-scale structure.
Open sectionHow matter is organized by gravity on large scales: planets, stars, stellar systems, galaxies, compact objects, and the evolving Universe.

Gas and dust → planets and stars → stellar systems → galaxies → large-scale structure.
Open sectionGravity compresses gas; nuclear reactions power stars; mass largely determines their later evolution.
Open sectionThe early Universe, stellar fusion and neutron-capture processes create the chemical elements.
Open section
The same physical laws connect structures over an enormous range of characteristic sizes.
Open section
A domain where KOINOT presents the standard picture and the CTPA interpretation side by side.
Open sectionExpansion, cosmic history, formation of structure, and the major open questions of cosmology.
Open section