Home Topics Data & Inference
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Key idea: This demo makes the full causal chain legible: Earth moves, line-of-sight changes, and the target star appears to shift against fixed backgr
This demo makes the full causal chain legible: Earth moves, line-of-sight changes, and the target star appears to shift against fixed backgr
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Key idea: Explore how relative motion shifts spectral lines and why astronomers can measure radial velocity from light alone.
Explore how relative motion shifts spectral lines and why astronomers can measure radial velocity from light alone.
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Key idea: Star formation does not make one star at a time. It makes a population, and the distribution of masses in that population — the initial mass
Star formation does not make one star at a time. It makes a population, and the distribution of masses in that population — the initial mass
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Key idea: Explore why spiral-galaxy rotation curves stay nearly flat at large radius and what that implies about dark matter across scales.
Explore why spiral-galaxy rotation curves stay nearly flat at large radius and what that implies about dark matter across scales.
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Key concepts
Learning goals aggregated from all exhibits in this topic.
Describe the initial mass function as a distribution, and state that low-mass stars dominate by number. Explain why the most massive star in a cluster varies a lot between clusters of the same size. Read a cluster's age from the main-sequence turnoff. Distinguish a model's output from the range over which the model is valid. Relate radial motion to observed wavelength and frequency shifts in spectral lines. Interpret redshift z and convert between z and radial velocity with the correct formula. Decide when non-relativistic Doppler is acceptable and when relativistic Doppler is required. Use lab-vs-observed spectral comparisons to infer motion direction and speed. Interpret galaxy rotation curves as velocity-versus-radius observables inferred from Doppler measurements. Compare visible-matter-only Keplerian predictions to flat observed curves and infer missing mass. Relate bulge, disk, and halo component models to total curve shape and enclosed-mass growth. Use baryon fraction and dark-to-visible ratio readouts to reason about mass budgets at large radius. Trace causality: Earth moves in orbit, line-of-sight changes, apparent star position shifts. Infer parallax from two captures using measured shift and effective baseline. Connect smaller inferred parallax to larger inferred distance. Describe why uncertainty and weak baseline geometry limit inference quality.