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exoplanetas
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Stellar Brief: 22. 10. 2026
A young, planet-hosting star called V1298 Tauri is showing how fiercely active infant planetary systems can be: radio emissions appeared in 90 percent of monitoring visits, while its X-ray brightness also changed and showed a stellar flare.
Read today's Stellar Brief
Latest astronomy noticias
17. 3. 2026
Estrellas | ExoplaneA new study has analysed six planetary systems, each with at least one small planet passing in front of its star. By combining new and existing observations from space and ground-based telescopes, researchers have measured the mass and size of these planets with high precision. This allows for a better understanding of what these distant worlds are made of and how they might have formed.
The team used data from CHEOPS, K2, TESS, and several ground-based observatories, along with radial veloci...
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17. 3. 2026The TOLIMAN mission is building and preparing to launch a low-cost space telescope with a unique optical design. Its main goal is to search for rocky, Earth-like planets in temperate orbits around the stars Alpha Centauri A and B, the closest Sun-like stars to Earth. Finding such planets is difficult with current instruments, even though these stars are nearby and bright.
TOLIMAN will use a technique called narrow-angle astrometry, which measu...
Read article 17. 3. 2026Estrellas | ExoplaneTOI-3884 b is a rare super-Neptune planet that transits a fully convective M-dwarf star with a persistent giant polar starspot. Because the planet passes over this spot during every transit, astronomers can directly study the spot’s properties using the James Webb Space Telescope (JWST). Seven transits were observed with JWST, covering a wide range of wavelengths from 0.5 to 5.3 micrometers.
Each transit showed a recurring signature as the pla...
Read article 16. 3. 2026Estrellas | ExoplaneSilicate clouds are a key feature in the atmospheres of many giant exoplanets, but their formation and composition are still being studied. This research compares the silicate clouds seen in four hot Jupiters observed by JWST with theories developed for brown dwarfs, objects that are between planets and stars in mass and temperature. The study also uses evidence from meteorites to show that giant planets forming in the outer regions of protoplane...
Read article 16. 3. 2026Estrellas | Exoplanetas | TESS | Enanas roj
The Neptunian desert is a region where Neptune-sized planets are rare at short orbital periods, likely due to intense starlight stripping away their atmospheres or changes in their orbits. Understanding this desert helps scientists learn how planets evolve, especially around different types of stars. In this study, astronomers confirmed the existence of TOI-672 b, a massive super-Neptune orbiting a red dwarf star, using data from TESS, ground-bas...
Read article 16. 3. 2026Estrellas | ExoplaneThe exoALMA Large Program has uncovered many detailed structures in the dust and gas of protoplanetary disks, where planets are forming around young stars. By using a technique called tomography—studying how molecular lines change at different locations and velocities—astronomers can now detect the presence of planets hidden within these disks.
The study shows that even with a few hours of ALMA telescope time, it is possible to spot the signat...
Read article 16. 3. 2026Estrellas | Exoplanetas | Telescopio espacial James Webb | Atmósferas planetariThe James Webb Space Telescope (JWST) has detected silicate clouds in the atmospheres of several exoplanets, providing new insights into how clouds form in extreme environments. While simple models can fit these observations, they do not always match the results from more detailed microphysical models. To address this, researchers developed Nimbus, a fast model that simulates cloud formation based on physical processes, and used it alongside Virg...
Read article 16. 3. 2026Estrellas | ExoplaneThe protoplanetary disk around TW Hya is a key site for studying how planets form and what materials they inherit. Understanding the distribution of chemical elements and molecules in such disks helps scientists learn about the building blocks of planets, especially those that could be habitable. One important molecule is formaldehyde (H2CO), which exists in two forms: ortho and para, depending on the spins of its hydrogen atoms.
Recent ALMA o...
Read article 13. 3. 2026Estrellas | ExoplaneLong-period giant planets, or cold Jupiters, play a key role in shaping planetary systems, but they are difficult to detect because they orbit far from their stars. Traditional methods like radial velocity and transit surveys have limited sensitivity at these distances. By combining long-term radial velocity data with precise astrometry from the Hipparcos and Gaia missions, astronomers can now better detect and measure these distant worlds.
In...
Read article 13. 3. 2026Estrellas | Exoplanetas | Atmósferas planetarias | Telescopio espacial James WebbWASP-107 b is a warm gas giant planet that has been studied in detail using the James Webb Space Telescope (JWST). Its atmosphere shows a unique feature at 8–10 micrometers, thought to be caused by silicate clouds. Scientists aimed to explain the planet’s full spectrum, from near-infrared to mid-infrared, using a physically realistic model of cloud formation and temperature.
The research team used a model that links how clouds form with how he...
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Exoplanetas recién descubiertos
| EK Chamaeleontis b | 10 / 2026 | 2702.2 M⊕ | 321.3 ly | |
| HD 715 b | 10 / 2026 | 201.9 M⊕ | 542.8 ly | |
| DENIS J1253-5709 b | 10 / 2026 | 244.8 M⊕ | 54.4 ly | |
| L 115-21 b | 10 / 2026 | 0.4 M⊕ | 41.9 ly | |
| TIC 219893931 b | 09 / 2026 | 8.9 M⊕ | 1319.5 ly | |
| TOI-6417 b | 09 / 2026 | 349.7 M⊕ | 1903.9 ly | |
| TOI-6443 b | 09 / 2026 | 1605.4 M⊕ | 2051.6 ly | |
| TOI-7219 b | 09 / 2026 | 661 M⊕ | 1074.2 ly | |
| TOI-4079 B b | 09 / 2026 | 1646.8 M⊕ | 1185.6 ly | |
| HD 45652 b | 09 / 2026 | 1557.7 M⊕ | 113.9 ly | |
| LSPM J0804+1116 b | 09 / 2026 | 6.4 M⊕ | 82.6 ly | |
| HR 8799 f | 09 / 2026 | 524.5 M⊕ | 133.3 ly | |
| 61 Cygni A b | 09 / 2026 | 2543.3 M⊕ | 11.4 ly | |
| TOI-5646 b | 08 / 2026 | 45.9 M⊕ | 1352.3 ly | |
| TOI-4468 c | 08 / 2026 | 11.1 M⊕ | 1233.1 ly |
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