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Astronomy: explore STEM content (page 24 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.
Looking Up Through History For most of human history, people had only their eyes to study the sky. A few curious thinkers changed forever how we understand our place in the universe. A Slow Change of Mind Big ideas in science rarely change
Astronomy
Astronomy · L1 · Astronomers Who Changed How We See the Sky
What physically causes a Cepheid variable to pulsate?1 / 8
Cepheids pulsate due to the kappa (κ) mechanism: in a particular temperature zone within the star (where helium is partially ionised), the gas's opacity increases as it is compressed, rather than decreasing as it normally would. This traps radiation, driving further expansion, which then decreases opacity and lets radiation escape, causing the star to contract again — a self-sustaining pulsation cycle rather than a one-off event.
Variable stars: Cepheids, RR Lyrae, and asteroseismology Some stars do not shine at constant brightness — they pulsate, rhythmically expanding and contracting. Two classes of these pulsating variables, Cepheids and RR Lyrae stars, are among
Three Kinds of Leftovers Not everything orbiting the Sun is a planet or moon. The solar system is full of smaller bodies — leftover material from its formation 4.6 billion years ago — and they come in a few distinct types. Why Comets Grow T
Astronomy
Astronomy · L2 · Comets, Asteroids, and Meteoroids
Interactive Astronomy Plots The Astronomy Visualised collection contains interactive graphs that let you explore fundamental astronomical relationships by adjusting parameters in real time. Hubble's Law The Hubble Law plot shows recession v
Astronomy
Astronomy · L3 · Interactive Astronomy: Exploring the Universe with Graphs
An active galactic nucleus is powered primarily by:
ANuclear fusion in a dense cluster of young starsBGravitational energy released as matter accretes onto a supermassive black holeCCollisions between galaxy clustersDRadioactive decay of heavy elements in the galactic core
AThe galaxy has less mass than it appears toBThere is more unseen mass than the visible matter alone accounts forCNewtonian gravity is completely wrongDThe galaxy is not actually rotating
One Data Point Is Not a Trend Until 1995, the only planetary system available to study was our own — eight planets on nearly circular orbits, rocky worlds close to the Sun and gas giants far out, with a wide, empty gap between them. Theorie
What is a mean-motion resonance between two orbiting bodies?1 / 8
A situation where two bodies' orbital periods form a ratio of small whole numbers (for example 2:1 or 3:2), so their relative alignment repeats in a fixed, predictable pattern on every cycle — producing a small gravitational tug that repeats at the same orbital phase every time, rather than averaging away as it would at a random, non-resonant period ratio.
Astronomy
Astronomy · L4 · Orbital Resonances, Lagrange Points & the Restricted Three-Body Problem
In the ΛCDM hierarchical structure-formation picture, which forms first?
AThe largest structures (superclusters), which later fragmentBSmall dark matter halos, which subsequently merge into larger structuresCFully formed spiral galaxies, directly from the primordial gasDGalaxy clusters, simultaneously with the halos inside them
Two Very Different Orbits Not all satellites orbit at the same height, and the altitude a satellite flies at changes everything about how it behaves. A satellite in Low Earth Orbit (LEO), only a few hundred kilometres up, races around the p
The King of the Planets Jupiter is the fifth planet from the Sun and by far the largest. It is so massive that all the other planets combined could almost fit inside it. Unlike Earth, Jupiter has no solid ground. It is a giant ball of gas,