Kepler’s small planets may be too distant for us to learn more about them, but the measurements have told us that we can expect several small planets to be in orbit around cool stars in much closer parts of the Galaxy. If they are close enough, then we may be able to measure their masses to determine whether or not they are rocky, and we might even be able to go further and find out what they are really like.
OpenLearn - An introduction to exoplanets
Except for third party materials and otherwise, this content is made available under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 Licence, full copyright detail can be found in the acknowledgements section. Please see full copyright statement for details.