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Astronomy: explore STEM content (page 25 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.
Radiative Transfer and Line Formation A stellar spectrum results from radiative transfer through an atmosphere with a temperature gradient: continuum photons escape from progressively shallower (cooler) depths as one moves to wavelengths wh
Astronomy
Astronomy · L5 · Spectral Line Formation, the Curve of Growth, and Non-LTE Effects
Five Ideas That Rewrote the Universe The history of astronomy is not a smooth accumulation of facts — it is a sequence of paradigm shifts, each one overturning the model that came before it once the evidence made the old picture untenable.
Astronomy
Astronomy · L3 · History of Astronomy: Paradigm Shifts
By mass, the interstellar medium is composed mostly of:
ADust grains, with a small amount of gasBGas (mostly hydrogen), with dust making up only about 1% by massCEqual parts gas and dustDHeavy elements like iron and gold
Fixing a Position on the Sky Just as any point on Earth can be located with longitude and latitude, any point on the sky can be located with the equatorial coordinate system: right ascension and declination. The celestial equator is simply
The practice of comparing planets to each other to understand why they turned out the way they did — and what that reveals about the rules governing all planets.
Exploring the Red Planet with Robots Mars is too far and too harsh for people to visit safely right now, so scientists send robotic rovers instead. These machines drive across the Martian surface, taking photos and testing rocks and soil. W
Two Competing Formation Channels Giant planets can, in principle, form via two very different physical processes, operating on very different timescales and favouring different disk conditions: What Kepler-Era Demographics Add Large transit
Astronomy
Astronomy · L5 · Planet Formation Channels and What Exoplanet Demographics Reveal
Protostellar evolution: from collapse to the main sequence Between the onset of a molecular cloud's gravitational collapse and a star's arrival on the stable main sequence lies a sequence of distinct observational stages, classified by how
Astronomy
Astronomy · L4 · Protostellar Evolution: From Collapse to the Main Sequence
Where Could Life Exist? The search for life beyond Earth starts with a simple question: where could liquid water exist on a planet's surface? That range of orbital distances around a star is called the habitable zone. A star's luminosity se
Astronomy
Astronomy · L3 · Habitable Zones & the Search for Life
The range of orbital distances from a star where a planet's temperature could allow liquid water to exist on its surface — not so close that water boils away, not so far that it freezes solid.
Astronomy
Astronomy · L3 · Habitable Zones & the Search for Life