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Solar-like oscillations are excited in cool stars with convective envelopesand provide a powerful tool to constrain fundamental stellar properties andinterior physics. We provide a brief history of the detection of solar-likeoscillations, focusing in particular on the space-based photometry revolutionstarted by the CoRoT and Kepler Missions. We then discuss some of the lessonslearned from these missions, and highlight the continued importance of smallerspace telescopes such as BRITE constellation to characterize very bright starswith independent observational constraints. As an example, we use BRITEobservations to measure a tentative surface rotation period of 28.3+/-0.5 daysfor alpha Cen A, which has so far been poorly constrained. We also discuss theexpected yields of solar-like oscillators from the TESS Mission, demonstratingthat TESS will complement Kepler by discovering oscillations in a large numberof nearby subgiants, and present first detections of oscillations in TESSexoplanet host stars.

Solar-Like Oscillations: Lessons Learned & First Results from TESS