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Astronomy: explore STEM content (page 16 of 26) · openstem
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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.
Supernova classification: light curves and spectral types Supernovae are classified observationally, by spectrum and light-curve shape, using a scheme that predates a full understanding of the underlying physics. As a result, the classifica
The tiny apparent shift in a nearby star's position against distant background stars, seen from two different points in Earth's orbit around the Sun (typically six months apart).
Two Kinds of Shadow Any object blocking a light source casts a shadow with two distinct parts: an umbra, the fully dark region where the light source is completely blocked, and a penumbra, the surrounding region where the light source is on
Astronomy
Astronomy · L2 · Eclipse Mechanics: Umbra, Penumbra, and Types
From Impact to Crater When an asteroid strikes a planet's surface at tens of kilometres per second, its enormous kinetic energy, is dumped into the ground almost instantaneously, driving crater formation through three distinct stages. The C
What holds up a neutron star against further gravitational collapse?
AOrdinary gas pressure from heatBNeutron degeneracy pressure, a quantum-mechanical effectCMagnetic repulsionDNothing — neutron stars are still collapsing
What does it mean for a planet to be in its star's habitable zone?
AThe planet definitely has life on itBThe planet's orbital distance would allow liquid water to exist on its surface, given the right conditionsCThe planet is the same size as EarthDThe star is the same type as the Sun
Astronomy
Astronomy · L3 · Habitable Zones & the Search for Life
The Tidal Radius and the Hills Mass A star is tidally disrupted once its pericenter distance falls inside the tidal radius, where the black hole's differential gravity across the star overwhelms the star's self-gravity: Because r_t grows on
Astronomy
Astronomy · L5 · Tidal Disruption Events: From Stellar Shredding to Observed Flares
Pictures Made of Stars On a clear night, the sky is full of stars. For thousands of years, people have connected some of those stars into imaginary pictures called constellations — animals, heroes, and objects from their stories. The stars
State the diffraction-limited angular resolution of a single dish, and explain why this is a much harder problem for radio telescopes than optical ones.1 / 9
The diffraction limit is θ ≈ 1.22λ/D, where λ is the observing wavelength and D is the dish diameter. Radio wavelengths (millimetres to metres) are 10⁴–10⁷ times longer than optical wavelengths (hundreds of nanometres), so for the SAME angular resolution, a radio telescope needs a correspondingly larger diameter than an optical one — reaching optical-telescope-like resolution with a single radio dish would require an impractically enormous structure.
Astronomy
Astronomy · L4 · Radio Astronomy: Single Dishes, Interferometry & the EHT
Two Puzzles in Standard Big Bang Cosmology Extrapolating the FLRW/Friedmann description of the universe back toward the Big Bang, without any exotic early-universe physics, leaves two well-posed puzzles that are not contradictions but natur
Astronomy
Astronomy · L5 · Cosmic Inflation: Solving the Horizon and Flatness Problems
What Is Light Pollution? Light pollution is excessive or misdirected artificial light that brightens the night sky far beyond its natural darkness. It comes from streetlights, buildings, signs, and homes — especially fixtures that send ligh
If gravity is always pulling planets toward the Sun, why don't they fall in?1 / 8
Planets are also moving sideways very fast. Gravity constantly bends that sideways motion into a curve, but the planet keeps moving forward fast enough to 'miss' the Sun over and over — that continuous falling-and-missing is an orbit.
What does it mean to say 'space itself is expanding,' as opposed to 'galaxies are moving through a fixed space'?
AGalaxies are physically flying apart at high speed under their own enginesBThe space between galaxies is stretching, carrying them apart much like dots on an inflating balloonCNothing is actually moving; it is an optical illusionDGalaxies are falling into a central point
The Highest-Energy Particles Known Ultra-high-energy cosmic rays (UHECRs) — almost always protons or atomic nuclei — carry energies above roughly 10^18-10^19 eV, with the most extreme detected events exceeding 10^20 eV concentrated into a s