Astronomers have announced the discovery of a third exoplanet orbiting Beta Pictoris, a young nearby star that has become a benchmark for directly imaging worlds beyond our Solar System. The newly confirmed planet, named Beta Pictoris d, is extraordinarily faint compared with the star’s brighter companions, yet its presence can be inferred from the subtle signatures hidden in old observations.
The planet was first spotted using the European Southern Observatory’s Very Large Telescope (VLT). Researchers then noticed something unusual: instead of a fresh, isolated detection, Beta Pictoris d appeared to have been “there all along,” concealed by the glare of Beta Pictoris b, the first planet found in the system.
By reanalyzing archive data collected over more than a decade, the team confirmed that the planet appears in multiple images, including cases where it is only barely visible against the dominant light of its neighboring planet. This approach turned a time-consuming hunting effort into a retrospective revelation, highlighting the value of long-term astronomical archives.
What makes Beta Pictoris d especially notable is its brightness and mass. The planet is about 100 times fainter than Beta Pictoris b and, based on its infrared properties and color, appears to be a gas giant with roughly 2.4 times Jupiter’s mass. Despite being larger than Earth but far lighter than many directly imaged giants, it ranks among the lightest exoplanets ever captured from the ground.
The system’s geometry also helps interpret the observations. In the processed VLT image, the host star was subtracted to reveal a debris disc viewed edge-on—an extended ring of material left over from planetary formation. The planet’s mass and orbital location align with the disc’s particular structure, offering a physical clue that connects the planet to the system’s history.
Direct imaging is difficult because a planet’s light is dwarfed by its star’s brightness. Detecting a world as faint as Beta Pictoris d required both sensitive instrumentation and careful data processing to separate planetary signals from noise and glare.
An independent team reported the same planet using the James Webb Space Telescope (JWST), providing independent confirmation across facilities and observing platforms. Together, the results strengthen confidence in the detection and provide complementary constraints on the planet’s properties.
With Beta Pictoris now serving as a rare multi-planet directly imaged system, researchers can compare multiple worlds forming in the same environment—an opportunity that can refine models of how planets grow and evolve.
The discovery also suggests that more faint planets may be hiding in existing datasets, awaiting the right analysis strategy. Upcoming next-generation telescopes may be able to reveal additional low-mass companions that have so far remained invisible.
Subject of Research: Direct imaging of exoplanets in the Beta Pictoris system
Article Title: Discovery of Beta Pictoris d (third planet in the system)
News Publication Date: Not specified in the provided text
Web References: https://doi.org/10.3847/2041-8213/ae80a0
References: The Astrophysical Journal Letters (DOI: 10.3847/2041-8213/ae80a0)
Image Credits: ESO/B. Sutlieff, M. Bonse et al.
Keywords
Exoplanets; Beta Pictoris; direct imaging; VLT/ERIS; JWST; gas giant; archival data; debris disc
