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Astronomy: explore STEM content (page 18 of 26) · openstem
Explore STEM Content
Search the community's STEM library — free to study, yours to make your own.
Astronomy
Stars, orbits, cosmology and observation on openstem — flashcards, notes, quizzes and plots shared by the community. Study free, or clone anything into your library.
Active galactic nuclei: accretion disks, jets, and supermassive black holes At the centre of most large galaxies sits a supermassive black hole (SMBH), typically millions to billions of solar masses. Most of the time this SMBH is quiescent,
Astronomy
Astronomy · L4 · Active galactic nuclei: accretion disks, jets, and supermassive black holes
Leftovers From Building the Solar System Not everything in space is a planet, a moon, or a star. Space is full of smaller rocky and icy objects — leftover pieces from when the solar system was forming billions of years ago. How a Comet Grow
State the (static, non-expanding) Jeans instability criterion and the Jeans length.1 / 8
In a static self-gravitating gas, pressure support competes with gravity; a perturbation collapses only if it is larger than the Jeans length, at which pressure forces can no longer respond fast enough to counteract gravitational collapse:
Kilometres Stop Being Useful A kilometre works fine for measuring a road trip. But space is so vast that using kilometres for it quickly produces numbers too large to picture — hence astronomers use two special units built for the job. Stac
Venus, Earth, and Mars formed in roughly the same region of the solar system from similar materials. What does comparative planetology try to explain?
AWhy they ended up so different despite similar starting pointsBWhy all three planets are actually identicalCHow many moons each planet hasDThe exact order the planets formed in
Nuclear fusion — hydrogen nuclei fuse into helium under crushing pressure and heat of about 15 million °C, releasing the energy that powers the entire Sun.
What are the two main classes of stellar oscillation modes, and what restoring force distinguishes each?1 / 9
Pressure modes (p-modes) are acoustic waves restored by pressure gradients — essentially trapped sound waves. Gravity modes (g-modes) are restored by buoyancy in a stably (radiatively) stratified region, oscillating as displaced fluid parcels are pushed back toward equilibrium by their density contrast with the surroundings.
Falling Around, Not Falling In It seems strange that gravity pulls planets toward the Sun all the time, yet they never crash into it. The trick is that planets are also moving sideways, fast. Gravity bends that sideways motion into a curve