This website does readability filtering of other pages. All styles, scripts, forms and ads are stripped. If you want your website excluded or have other feedback, use this form.

Stars, Planets and Origins |

Skip to main content area

Stars, Planets and Origins

When we look up at the sky at night, we see light produced by stars. The Moon and the planets shine by reflected starlight. The light from distant galaxies is the light from hundreds of billions of stars. Stars form in large clouds of gas and dust. Planets grow in the circumstellar disk that surrounds every newborn star. To learn how stars form, CfA scientists study the structure of dark clouds and the young stars within the clouds. To study the birth of planets, CfA scientists examine the structure of circumstellar disks and outflowing jets associated with the youngest stars. Once a star is mature, its brightness is fairly steady for hundreds of millions to tens billions of years. This steadiness allows planets orbiting a star to develop stable surfaces that might allow life to develop and perhaps flourish. CfA scientists study the structure and evolution of stable (and unstable stars) and search for planets orbiting around them.

Accretion Disks (SSP) Asteroseismology (SSP) Binary Stars (SSP) Brown Dwarfs (RG) Circumstellar Disks and Planet Formation (RG) Computational Stellar Astrophysics (HEA) Dense Cloud Cores (RG) Dynamical Architecture of Planetary Systems (TA) Early-type Stars (HEA) Embedded Clusters (RG) Evolved Stars (RG) Giant Magellan Telescope (OIR) Hypervelocity Stars (OIR) Kozai-Lidov Mechanism (TA) Laser Frequency Combs for Astrophysics (astro-combs) (AMP) Late-Type Stars and Brown Dwarfs (AMP) Life and the Cosmos (HEA) Magnetohydrodynamic Effects in Hot Planetary Atmospheres; (TA) Massive Star Formation (RG) Merging White Dwarfs (OIR) Milky Way Halo (OIR) Molecular Clouds (RG) Open Clusters (OIR) Planet Formation (SSP) Planetary Dynamics and Celestial Mechanics (TA) Planetary Nebulae (OIR) Resonance Overlap and Planetary Stability (TA) Star Formation (OIR) Star Formation (SSP) Star Formation (HEA) Stellar Atmospheres (SSP) Stellar Corona (HEA) Stellar Coronae/Winds (SSP) Stellar Variability (SSP) Supernovae (OIR) The Origins of Stellar Spin - Planetary Orbit Misalignments (TA) Time Domain Astrophysics (HEA) Transit Timing Variations (TA) Ultracool Stellar Magnetism (OIR) White Dwarfs and Novae (HEA) Young Stellar Objects (RG)


Submitted by rclinch-adm on May 8, 2012 - 4:01pm

Research By Division

Submitted by jshaw-adm on March 21, 2013 - 2:14pm