![The separation of β Pictoris b and β Pictoris c from the star in terms of their Hill sphere. β Pictoris b has a longer orbital period (∼20 yr), with a Hill sphere primary transit at MJD ∼58000 and a Hill sphere radius of 1.1 au. β Pictoris c has a shorter orbital period (∼3.3 yr), with two primary transits at MJD 58195+11 −20 and 59415+8 −8 and a secondary transit at 58707+3 −7 . The § Hill sphere radius is approximately 0.3 au. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/The-Hill.png?resize=1200%2C712&ssl=1)
[astro-ph.EP]. Beta Pictoris is a young and nearby planetary system hosting an edge-on debris disk and at least three gas-giant planets. Their circumplanetary environments could host exomoons and rings, a […]
Beta PIctoris
Posted inBeta Pictoris
Webb Discovers A Hidden Planet In The Beta Pictoris Star System
[NASA] Astronomers using NASA’s James Webb Space Telescope have discovered a giant planet outside our solar system, called an exoplanet, hiding within one of the most intensely studied planetary systems […]
Posted inBeta Pictoris
Exoplanet Beta Pictoris d Found After More Than 10 Years Of Searching
[ESO] A team of astronomers have discovered a third planet orbiting the star Beta Pictoris. The new planet, Beta Pictoris d, is 100 times fainter than Beta Pictoris b — […]
Posted inAstrochemistry, Atmospheres, Climate, Weather, Beta Pictoris, Exoplanets, -moons, -comets, Icy Worlds, Imaging & Spectroscopy, Interstellar, Status Report
13CO And Potential Variability In β Pictoris b With GRAVITY+
The 12CO/13CO ratio was introduced as an indicator for where in the disk a planet has formed. Previously a lower value compared to the host star’s was suggested to show […]
Posted inAstrochemistry, Astronomy & Telescopes, Biosignatures & Paleobiology, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Interstellar, Status Report
The Carbon Isotope Ratio Of β Pic b With High-resolution Spectroscopy
Isotopic ratios trace the formation and evolution of planets and link their atmospheres to the chemistry of their natal protoplanetary discs.
Posted inAstrochemistry, Astrogeology, Astronomy & Telescopes, Beta Pictoris, Biochemistry & Organic Chemistry, Comets and Asteroids, Exoplanets, -moons, -comets, Icy Worlds, Imaging & Spectroscopy, Status Report
Observations Of Exocomets
Active small bodies in extrasolar systems, the extrasolar analogues of Solar System comets, provide insights into the orbital evolution and physical processes shaping planetary systems.
Posted inAstronomy & Telescopes, Beta Pictoris, Comets and Asteroids, Exoplanets, -moons, -comets, Icy Worlds, Imaging & Spectroscopy, Status Report
Visual Inspection Of Potential Exocomet Transits Identified Through Machine Learning And Statistical Methods
In this work, we explore several ways to detect possible exocomet transits in the TESS (The Transiting Exoplanet Survey Satellite) light curves. The first one has been presented in our […]
Posted inBeta Pictoris, Comets and Asteroids, Exoplanets, -moons, -comets, Icy Worlds, Imaging & Spectroscopy, Status Report
Transit Distances And Composition Of Low-velocity Exocomets In The β Pictoris System
β Pictoris is a young nearby A5V star, about 20 Myr old, embedded in a prominent debris disc. For the past 40 years, variable absorption features have been observed in […]
Posted inAstronomy & Telescopes, Beta Pictoris, Exoplanets, -moons, -comets, Status Report, Stellar Cartography
First Astrometric Limits On Binary Planets And Exomoons Orbiting β Pictoris b
The search for exomoons, or moons in other star systems, has attracted significant interest in recent years, driven both by advancements in detection sensitivity and by the expanding population of […]
![Distance versus time distributions for the 49 encounters with β Pic that have an empirical probability of at least 95% of occurring within 2 pc. The coloured points indicate the rescaled Mahalanobis distances (ensuring a common colour scale for all stars) derived from the encounter parameters. Points above the 95th percentile of this metric are shown in grey. The black bars represent the 95% confidence intervals in time and distance, obtained from the 2.5th and 97.5th percentiles of the corresponding marginal distributions for the further encounters and using the 95th percentile to define the one-tailed distance interval for the closest ones. The central points are the 50th percentiles. The critical radius of 2 pc is indicated by the red horizontal line. The centres of mass of binary systems, listed in table 4, are marked at the pair [t50, d50] corresponding to that star. -- astro-ph.SR](https://i0.wp.com/astrobiology.com/wp-content/uploads/2025/10/A-Kinematic-History-Of-Stellar.png?resize=1200%2C719&ssl=1)
Posted inBeta Pictoris, Exoplanets, -moons, -comets, Status Report, Stellar Cartography
A Kinematic History Of Stellar Encounters With Beta Pictoris
Beta Pictoris is an A-type star hosting a complex planetary system with two massive gas giants and a prominent debris disk.