Past exam of the mathematics course of the University of Cambridge 2026 iii Paper 315 3 a iii Solution Created 2026-09-24 Updated 2026-09-24
For a hot Jupiter transiting a Sun-sized star,a one-percent baseline transit. Taking , , and an -dominated mean molecular mass gives an atmospheric scale height near . A strong band spanning five scale heights then hasor several hundred parts per million; very strong clear-atmosphere features can approach . The spectrum is therefore a roughly one-percent baseline with a localized Gaussian-sized band near and a continuum rising toward short wavelengths when . Clouds reduce both and the observable power-law slope.
Past exam of the mathematics course of the University of Cambridge 2026 iii Paper 315 3 c iii Solution Created 2026-09-24 Updated 2026-09-24
For an Earth twin around the Sun, , , , givingFor a super-Earth with a heavy atmosphere around a M dwarf, take , givingFor a hydrogen-rich sub-Neptune around a star, take , , , and hence . ThenThe hydrogen-rich sub-Neptune is the most observable with JWST because its low molecular mass and large radius produce the largest transmission annulus. Clouds can reverse this ranking in a particular system.