Lloyd, J.P., Lunine, J.I., Mamajek, E., Spiegel, D.S., Covey, K.R., Shkolnik, E.L., Walkowicz, L., Chavez, M., Bertone, E., & Olmedo Aguilar, J.M.,
Targeting Young Stars with Kepler: Planet
Formation, Migration Mechanisms and the Early History of
Planetary Systems, eprint arXiv: 1309 - 1520, 2013
Young stars (only 100 million years old) are prime
targets for
planetary detection through imaging because the planets around them are still flush with the heat of their
formation and are therefore brighter.
Thanks to the proximity and the fact that its axis of rotation points roughly in the Earth's direction, giving us a face - on - view of the developing
planetary system, TW Hydrae is one of the most favorable
targets for investigating planet
formation.