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YORP Effect 3D Explorer vs Yarkovsky Effect 3D Explorer


Both pages teach a real, non-gravitational, sunlight-powered mechanism in one page load - 0 MB installed, USD 0, no account. The YORP Effect 3D Explorer covers the net torque that changes an asteroid's spin rate; the Yarkovsky Effect 3D Explorer covers the net force that shifts an asteroid's orbit instead.


The numbers side by side

AspectYarkovsky Effect ExplorerYORP Effect Explorer
Install size0 MB - runs in the browser0 MB - runs in the browser
PriceUSD 0USD 0
What changesthe orbit (semimajor axis)the spin rate
Real measured caseasteroid Bennu, -284.6 +/- 1.5 m/yearasteroid 54509 YORP, (2.0 +/- 0.2) x 10^-4 deg/day^2
Mechanismnet force from thermal-lag re-emissionnet torque from asymmetric-facet reflection/re-emission

Where the Yarkovsky Effect Explorer wins

The Yarkovsky Effect Explorer wins when the question is about how an asteroid's orbit itself drifts over time - the semimajor-axis change that matters for long-term impact-risk refinement, as it did for Bennu.


Where the YORP Effect Explorer wins

The YORP Effect Explorer wins when the question is about why an asteroid's rotation rate itself speeds up or slows down, and why that is a torque, not a force - it is the only page on the site with a torque-couple visualization and a spin-up/spin-down toggle.


A reasonable rule

As a reasonable rule, use the Yarkovsky Effect Explorer first to see how sunlight can quietly reshape an asteroid's orbit, then use the YORP Effect Explorer to learn the companion mechanism that reshapes the same body's spin instead.

See how to use the YORP Effect 3D Explorer for a step-by-step walkthrough.

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