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Planet Labs participated in the U.S. Department of Commerce commercial space trade mission to India.
Cheops observations revealed a fourth planet orbiting farther from LHS 1903 than the previously known three planets.
Measurements show that the innermost planet of LHS 1903 is rocky.
Planet provides daily, analysis-ready satellite data intended to support scalable insights, advanced predictive models, and global risk analysis for the insurance industry.
AXA Digital Commercial Platform (AXA DCP) will integrate data from Planet’s high-resolution and medium-resolution satellites and high-frequency Basemaps into its AI-powered platform.
The partnership will integrate Planet’s satellite data into AXA’s digital platform to enable smarter claims monitoring.
Ignacio Zuleta spent more than a decade working for or advising Planet Labs, Satellogic, and Hydrosat.
Planet’s satellite data is intended to support disaster preparedness, drought monitoring, and wildfire and flood risk assessment for insurers.
Space-based channels provide a low-loss path that enables long-distance quantum key distribution between remote points on the planet.
Planet’s near-daily global scan will enable AXA DCP to provide clients with a ground-truth layer of environmental intelligence for preventative action against extreme weather events.
Will Marshall is the CEO and Co-Founder of Planet Labs.
Europe's exoplanet-probing Cheops space telescope detected a fourth planet in the LHS 1903 system that is rocky and lies farther out than two gas giants in the system.
The planet ordering in the LHS 1903 system is rocky, gaseous, gaseous, and then rocky, creating an inside-out configuration.
The standard planet-formation theory holds that planets form simultaneously within a protoplanetary disc composed of gas and dust through coagulation of dust grains into planetary cores.
Isabel Rebollido is a planetary disc researcher at the European Space Agency who highlights that diverse exoplanet systems are prompting reassessment of traditional planet-formation theories.
The fourth planet orbiting LHS 1903 appears to have formed in a gas-depleted environment after the system had lost most of its protoplanetary gas.
The outer rocky planet in the LHS 1903 system likely formed when the system had already depleted its gas reservoir.
Cheops observations discovered a fourth small planet in the LHS 1903 system that is the most distant from the star and is rocky.
After excluding catastrophic impacts and planetary migration scenarios for LHS 1903, the preferred explanation is sequential planet formation rather than simultaneous formation from a single protoplanetary disk.
Cheops observations revealed that the outermost planet in the LHS 1903 system is rocky.