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Astronomy: explore STEM content (page 6 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.
AIt reflects starlight off its dust grainsBUltraviolet radiation from nearby hot stars ionises its gas, which then emits light as electrons recombineCIt is heated by cosmic ray bombardment aloneDIt glows from residual heat left over from the Big Bang
A Convergent, Multi-Scale Case for Dark Matter No single observation proves dark matter exists; rather, several independent lines of evidence — spanning galaxy, cluster, and cosmological scales, using entirely different physical mechanisms
Astronomy
Astronomy · L5 · Dark Matter: Evidence and Candidate Particles
What is the International Space Station (ISS)?1 / 7
A large research station orbiting about 400 km above Earth, built and operated by multiple countries. It has been continuously crewed by rotating astronaut teams since November 2000.
That the observable Universe began roughly 13.8 billion years ago from an extremely hot, dense state, and has been expanding and cooling ever since — not an explosion into pre-existing space, but an expansion of space itself.
Light Is More Than What We See Visible light is only a narrow slice of the full electromagnetic spectrum. Every band, from long-wavelength radio waves to extremely short-wavelength gamma rays, carries different information about the Univers
Why do different images of a strongly lensed quasar show the same brightness fluctuation at different times?
AEach image is actually a completely different, unrelated quasarBEach image's light follows a different path length and gravitational potential depth through the lensCThe quasar itself flickers independently in each directionDAtmospheric effects on Earth delay some images but not others
Collapse at Horizon Re-Entry Unlike an ordinary stellar-collapse black hole, a primordial black hole (PBH) forms directly from a sufficiently large density perturbation in the radiation-dominated early universe, at the instant that perturba
Astronomy
Astronomy · L5 · Primordial Black Holes: Formation and Dark-Matter Constraints
Four Seasons, One Tilted Earth Earth doesn't spin perfectly upright — its axis leans over by about 23.5 degrees. That single tilt is the reason we get four different seasons every year. As Earth travels around the Sun over the year, the til
AIt has oceans just like EarthBIt is close to Earth in size and made of similar rockCPeople can breathe its airDIt orbits the Sun at the same speed as Earth
Pushing Against Gravity Getting to space is hard because Earth's gravity holds on tight. A rocket has to move extremely fast — thousands of kilometres per hour — to break free and stay in orbit or head further out. To reach that speed, a ro
AA group of stars that formed together and are held together by gravityBAny two stars that happen to appear close together from EarthCA single star that is unusually brightDA cluster of planets orbiting one star
What is the Eddington luminosity, and where does its formula come from?1 / 8
The Eddington luminosity is the maximum luminosity at which outward radiation pressure on ionised gas balances inward gravity for spherical accretion (or, more loosely, sets a characteristic scale for disk accretion). Balancing radiation pressure on free electrons (via Thomson scattering, cross-section σ_T) against gravity on the associated protons gives:
What was Ptolemy's geocentric model, and how did it explain retrograde motion?1 / 8
A model, dominant for roughly 1400 years, in which Earth sits motionless at the centre of the universe and everything else orbits it. To explain planets occasionally appearing to move backward (retrograde motion), Ptolemy added epicycles — small circular loops layered on top of the main orbital circle.
Astronomy
Astronomy · L3 · History of Astronomy: Paradigm Shifts