English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Radial velocity surveys suggest that the Solar System may be unusual and thatJupiter-like planets have a frequency <20% around solar-type stars. However,they may be much more common in one of the closest associations in the solarneighbourhood. Young moving stellar groups are the best targets for directimaging of exoplanets and four massive Jupiter-like planets have been alreadydiscovered in the nearby young beta Pic Moving Group (BPMG) via high-contrastimaging, and four others were suggested via high precision astrometry by theEuropean Space Agency's Gaia satellite. Here we analyze 30 stars in BPMG andshow that 20 of them might potentially host a Jupiter-like planet as theirorbits would be stable. Considering incompleteness in observations, our resultssuggest that Jupiter-like planets may be more common than previously found. Thenext Gaia data release will likely confirm our prediction.

Jupiter-like planets might be common in a low-density environment