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Astronomy: explore STEM content (page 11 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.
Eyes That See Farther Our eyes are amazing, but they can only collect a small amount of light. A telescope has a much bigger opening — a lens or a mirror — that gathers far more light, letting us see things that are too small, too faint, or
What observational property is used to classify young stellar objects into Class 0 through III?
AThe star's total massBThe shape of its spectral energy distribution, tracing how much light escapes at shorter wavelengthsCThe number of planets already formed around itDIts distance from Earth
Astronomy
Astronomy · L4 · Protostellar Evolution: From Collapse to the Main Sequence
An unseen form of matter, inferred from its gravitational effects, that neither emits nor absorbs light — it does not interact with the electromagnetic force the way ordinary matter does.
Radio telescopes face a harder resolution problem than optical telescopes mainly because:
ARadio waves travel slower than lightBRadio wavelengths are far longer than optical wavelengths, so matching optical resolution needs a far larger dishCRadio dishes cannot be made reflective enoughDThe atmosphere blocks all radio wavelengths
Astronomy
Astronomy · L4 · Radio Interferometry & the EHT — 4 Q
What is proper motion, and what does it directly measure?1 / 8
A star's observed angular rate of motion across the sky, measured in arcseconds per year. It captures only the component of the star's true velocity that is perpendicular to the line of sight — its plane-of-sky, or 'tangential,' motion — and says nothing on its own about motion toward or away from the observer.
What is relativistic beaming, and what causes it?1 / 8
The concentration of radiation from a source moving at a speed close to the speed of light into a narrow cone in the direction of motion, as seen by a stationary observer. It arises from the relativistic aberration of light: in the source's own rest frame, emission may be nearly isotropic, but transforming to the observer's frame sweeps that radiation forward into a tight beam of half-angle roughly 1/Γ, where Γ is the bulk Lorentz factor of the jet.
Relativistic Beaming A source moving at a bulk Lorentz factor Γ close to the speed of light does not radiate isotropically as seen by a stationary observer, even if it does so in its own rest frame. Relativistic aberration sweeps that emiss
The Ringed Planet Saturn is the sixth planet from the Sun, and it is best known for the wide, bright rings that circle around it. Through a small telescope, Saturn's rings are one of the most amazing sights in the night sky. Like Jupiter, S