The idea of magnetism atmosphere on planet-forming isn’t new. It’s the first time it has been linked of the mystery of the observed excess infrared light. The planet-forming disks, which circle the young stars heat up by starlight, and glows with infrared light. A theory on planet-forming disks suggesting answers: Gas and dust suspend the disks above on gigantic loops seen of the sun absorb sunlight, and glow infrared light. The stars around the planet-forming material makes its way into future planets, asteroids, and comets. Magnetism atmospheres are similar to taking  place on the surface of our sun, which magnetic moving field lines spur huge solar prominences flaring up in big loops. It became clear disks aren’t enough to account the extra infrared light, even of stars a few times the mass of the sun. Stars surrounded a giant dusty halo, then intercepts the star’s visible light and re-radiated at infrared wavelengths. The result is that the atmosphere absorbs and re-radiates much to account all the extra infrared light. The starlight intercepts material not in a halo, and not inside a traditional disk, but in a disk atmosphere, which is supported by magnetic fields.