k-dense-ai/planetary-scientist
v1.1.0MIT
Reasons from bulk density, moment of inertia, tidal Love numbers, libration, electromagnetic induction, and sample-calibrated impact-flux chronology through NAIF SPICE kernels, PDS4 archives, radio-science gravity with SHTOOLS, PSG/NEMESIS retrievals, gamma-ray/neutron and radar sounding, and COSPAR planetary-protection categories while treating non-hydrostatic shapes, plasma currents mimicking ocean induction, radar clutter and roughness mimicking ice, single-line trace-gas detections, and one-flyby snapshot bias as first-class failure modes.
What this package declares
The file a client reads when it loads this plugin, exactly as this revision carries it.
plugin.json
{
"$schema": "https://agent-plugins.org/schemas/1.0.0/plugin.schema.json",
"name": "planetary-scientist",
"version": "1.1.0",
"description": "Reasons from bulk density, moment of inertia, tidal Love numbers, libration, electromagnetic induction, and sample-calibrated impact-flux chronology through NAIF SPICE kernels, PDS4 archives, radio-science gravity with SHTOOLS, PSG/NEMESIS retrievals, gamma-ray/neutron and radar sounding, and COSPAR planetary-protection categories while treating non-hydrostatic shapes, plasma currents mimicking ocean induction, radar clutter and roughness mimicking ice, single-line trace-gas detections, and one-flyby snapshot bias as first-class failure modes.",
"author": {
"name": "K-Dense",
"url": "https://www.k-dense.ai"
},
"homepage": "https://github.com/K-Dense-AI/scientific-agents",
"repository": "https://github.com/K-Dense-AI/scientific-agents",
"license": "MIT",
"keywords": [
"science",
"agents-md",
"expert-profile",
"planetary-scientist"
]
}