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This page contains a summary of the current calendar year's Exoplanet Archive news. For other news archives by year, see the 2025, 2024, 2023, 2022, 2021, 2020, 2019, 2018, 2017, 2016, 2015, 2014, 2013, and 2011-12 archives.
To view only the most recently added planets and updated parameters (default and non-default), see this pre-filtered and pre-sorted interactive table.
This week's update features TOI-4507 b, one of the longest-period and youngest "super-puff" planets confirmed to date. The other new planets are KMT-2024-BLG-1005L b, NGTS-34 b, NGTS-35 b, TOI-3288 b, TOI-4666 b, TOI-4940 b, TOI-5349 b, and TOI-7166 b.
Click on a planet name to go directly to its System Overview page, or browse the Planetary Systems and Planetary Systems Composite Data tables.
There are also six new JWST spectra for LTT 3780 b added to the Atmospheric Spectroscopy Table.
News panel image credit: NASA, ESA, and L. Hustak, J. Olmsted, D. Player and F. Summers (STScI)
We're kicking off 2026 with seven new planets, one demotion, one spectrum, and a gaggle of parameters that were submitted using our new template, now available through the Published Data Upload service!
The new planets are HD 128717 b, V2376 Ori b, TOI-5489 b & c, TOI-5716 b, TOI-5728 b, and TOI-5736 b. There are also new parameters for HD 143811 b, HAT-P-5 b, HAT-P-8 b, HAT-P-13 b, HAT-P-15 b, HAT-P-16 b, HAT-P-17 b, HAT-P-21 b, HAT-P-26 b, HAT-P-29 b, KELT-16 b, TIC 118798035 b, c & d, WASP-4 b, WASP-19 b, WASP-21 b, WASP-44 b, WASP-52 b, and WASP-103 b. Click on a planet name to go directly to its System Overview page, or browse the Planetary Systems and Planetary Systems Composite Data tables.
Kepler-1658 b's disposition had been updated to False Positive Planet (FPP) based on a published refutation. FPP data are removed from the Planetary Systems and Planetary Systems Composite Parameters tables, but are still available on the System Overview pages.
We've also added a new HD 143811 b spectrum taken by the Gemini Planet Imager (GPI) to the Atmospheric Spectroscopy Table.