Discovering an exoplanet doesn’t mean having one, definitive eureka moment. Instead, it requires multiple observations, sometimes from multiple observatories, and the scientific community coming together in agreement to finally confirm […]
Kepler
An Eccentric Sub-Neptune Moving Into the Evaporation Desert
Though missions such as Kepler, K2, and TESS have discovered >2,000 sub-Neptune and Neptunian planets, there is a dearth of such planets at close-in (P≲3 days) orbits.
TESS Investigation -Demographics of Young Exoplanets (TI-DYE) III: An Inner Super-Earth In TOI-2076
Young (<500 Myr) multi-planet transiting systems are valuable environments for understanding planet evolution by offering an opportunity to make direct comparisons between planets from the same formation conditions.
Search For Exoplanetary Ring Systems With TESS
Photometric surveys for exoplanetary ring systems have not confirmed any object with Saturn-sized ring.
Searching for Additional Planets in TESS Multi-Planet Systems: Testing Empirical Models Based on Kepler Data
Multi-planet system architectures are frequently used to constrain possible formation and evolutionary pathways of observed exoplanets.
Numerical Simulations Of The Interaction Between The Stellar Magnetic Field And A Planet
Kepler and TESS observations led to the discovery of many close-in super Earths, including some with ultra-short orbital periods (≲1 day).
Comparing The Sun To Sun-like Stars. On The Importance Of Addressing Faculae/spot Domination
Whether the Sun is an ordinary G-type star is still an open scientific question.
A Homogeneous Catalog of Oscillating Solar-Type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity
We present a homogeneous catalog of global asteroseismic parameters and derived stellar parameters for 765 Kepler main-sequence and subgiant stars.
Signatures of Atmospheric Mass Loss and Planet Migration in the Time Evolution of Short-Period Transiting Exoplanets
Comparative studies of young and old exoplanet populations offer a glimpse into how planets may form and evolve with time.
Small And Large Planets Have Significantly Different Upbringings
The shape of a planet’s orbit is one of its fundamental properties, along with its size and distance from its host star. Earth has a nearly circular orbit, but some […]
