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Astronomy: explore STEM content (page 23 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.
The cosmic microwave background: recombination, decoupling, and anisotropies The cosmic microwave background (CMB) is the oldest light astronomers can observe directly — a snapshot of the universe as it existed roughly 380,000 years after t
Astronomy
Astronomy · L4 · The cosmic microwave background: recombination, decoupling, and anisotropies
AA rocky planet with a thick, superheated atmosphereBA gas giant orbiting very close to its star, with a period of only daysCA giant planet ejected from its system entirelyDA planet with an unusually hot, molten core
Transmission spectroscopy detects an exoplanet's atmospheric composition by measuring:
AThe planet's total mass from its orbital wobbleBHow transit depth varies with wavelength, revealing wavelength-dependent atmospheric absorptionCThe planet's rotation period from its day-night temperature differenceDThe colour of reflected starlight only, with no wavelength dependence
Astronomy
Astronomy · L4 · Exoplanet Atmospheres & the Habitable Zone — 4 Q
Orbital resonances, Lagrange points, and the restricted three-body problem Beyond simple two-body orbits, gravitational interactions between three or more bodies produce two of the Solar System's most important recurring structures: mean-mo
Astronomy
Astronomy · L4 · Orbital Resonances, Lagrange Points & the Restricted Three-Body Problem
Bottom-Up Assembly in a CDM Universe In the ΛCDM paradigm, the small, nearly scale-invariant density perturbations seeded by inflation grow under gravity, with the smallest scales crossing the non-linear collapse threshold first. This produ
Astronomy
Astronomy · L5 · Hierarchical Structure Formation and Galaxy Assembly
An orbit roughly 160 to 2,000 km above Earth's surface, with an orbital period of about 90 minutes. The International Space Station and many imaging satellites use LEO.
A Star Built in Layers The Sun isn't a single uniform ball — it's built from distinct layers, each behaving differently as energy generated in the core works its way outward. The Corona's Strange Heat One of the Sun's biggest puzzles: the c
State the vis-viva equation and define every symbol in it.1 / 9
v² = GM(2/r − 1/a), where v is orbital speed at radius r, G is the gravitational constant, M is the central body's mass, r is the instantaneous distance from the focus, and a is the orbit's semi-major axis. It applies to any conic orbit (ellipse, parabola, hyperbola) once the correct sign and value of a are used.
Astronomy
Astronomy · L4 · Orbital Mechanics — Vis-Viva & Transfer Orbits
AA star's true speed through spaceBThe angular rate at which a star appears to move across the skyCA star's speed directly toward or away from the observerDA star's distance from Earth
What must happen inside a protostar for it to become a true main-sequence star?
AIts outer layers must cool completelyBIts core must reach about 10 million K and ignite sustained hydrogen fusionCIt must collide with another protostarDIt must lose most of its mass
Four Messengers, One Universe Multi-messenger astronomy combines fundamentally different carriers of astrophysical information, each sensitive to different physical conditions and each escaping its source under different circumstances: GW17
Astronomy
Astronomy · L5 · Multi-Messenger Astronomy: Gravitational Waves, Neutrinos, and Light from One Event