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Research draft

redshift

vr.tr.redshift · XCT.QLT

Let an agent explain redshift and its causes, relay measurement methods and their use in cosmology from astronomy references, describe key results such as Hubble s law, and distinguish redshift from blueshift, from reddening by dust and from the everyday sense of red colour.

Thing Registry Cross-cutting context

Research draft, second pass

A second pass drafted this model: the structure a model of this thing needs, and what is known about it in the world. The line under this one says how the second half was obtained - researched against sources, or recalled without web access, in which case nothing here was read anywhere and every claim is a lead to verify. Unreviewed either way.

written by Claude from model knowledge without web access - no source was read, every claim is a lead to verify

Researched by: Claude

Purpose and description

Let an agent explain redshift and its causes, relay measurement methods and their use in cosmology from astronomy references, describe key results such as Hubble s law, and distinguish redshift from blueshift, from reddening by dust and from the everyday sense of red colour.

The increase in wavelength of light or other radiation from a source, shifting spectral lines toward the red, caused by the source moving away in the Doppler effect, by the expansion of the universe in cosmological redshift, or by climbing out of a gravitational field in gravitational redshift, measured precisely from spectra as spectroscopic redshift or estimated from colours as photometric redshift; redshift is the main tool for measuring distances and the expansion of the universe.

What it is for: Measuring motion, distance and expansion.

It can be explain causes; relay measurement; describe cosmological use; distinguish related concepts.

Distinguishing features

Wavelength shift

Three causes

Distance proxy

Cosmology foundation

What it looks like

Not a visible object; spectral lines displaced toward longer wavelengths.

Physical character

definition: z = (observed minus emitted wavelength) over emitted formula

highest confirmed galaxy redshift: above 13 z - 2020s

CMB redshift: about 1100 z

Hubble s law: 1929 year

How it is recognised

Wavelength increase of light

Doppler, cosmological, gravitational; spectroscopic and photometric redshift

Blueshift is the opposite; dust reddening dims blue light without shifting lines

Related models

is a kind of - in registry terms

physical quantity

is caused by - for moving sources

Doppler effect

is used in - to measure expansion

Hubble s law

is contrasted with - a shift toward shorter wavelengths

blueshift

In practice

Families and kinds

Doppler redshift from motion

cosmological redshift from expansion

gravitational redshift

spectroscopic redshift measurement

photometric redshift estimation

redshift surveys of galaxies

Standards and regulation

No regulation; astronomical data standards for redshift catalogues

Failure modes and hazards

Confusing redshift with reddening

Treating cosmological redshift as a simple Doppler shift

Photometric redshift errors

Also called

spectroscopic redshiftcosmological redshiftphotometric redshiftgravitational redshift

Where this came from

wikidata · CC0 1.0

Drafted structure

Bundle to layer to finding to question, as the second pass will find it: 4 bundles · 8 layers · 8 findings · 16 questions.

Understand What redshift is.

Science.

Definition

Definition and causes.

Definition

Definition.

  1. What is redshift, and how do Doppler, cosmological and gravitational redshift differ from blueshift and dust reddening? definition
  2. Is the question about the concept, a cause, measurement or cosmology? boundary

Formula

Definition and scale.

Formula

Formula.

  1. How is z defined, and what do redshifts of 0.1, 1, 10 and 1100 mean? definition
  2. Which entry fits the cosmic distance ladder? action
Measure Measurement.

Practice.

Spectroscopic

Spectroscopic redshift.

Spectroscopic

Spectroscopic.

  1. How are redshifts measured from spectral lines? measurement
  2. Which references are standard? provenance

Photometric

Photometric redshift.

Photometric

Photometric.

  1. How are redshifts estimated from colours, and how accurate are they? measurement
  2. Which sources are cited? provenance
Cosmology Cosmology.

Science.

Expansion

Expansion.

Expansion

Expansion.

  1. How did Hubble and later surveys use redshift to establish and measure cosmic expansion? provenance
  2. Which entry fits the expansion of the universe? action

Surveys

Redshift surveys.

Surveys

Surveys.

  1. What have redshift surveys such as SDSS revealed about large-scale structure? provenance
  2. Which entry fits redshift survey? action
Context Gravity and history.

Context.

Gravity

Gravitational redshift.

Gravity

Gravity.

  1. How does gravitational redshift test general relativity, from Pound-Rebka to GPS? provenance
  2. Which entry fits tests of general relativity? action

History

History.

History

History.

  1. How was redshift discovered and interpreted by Slipher, Hubble and Lemaitre? provenance
  2. Which entry fits the history of cosmology? action

What the second pass must settle

  • Should cosmological and gravitational redshift be separate primary entries?
  • How should astronomy references be linked?
  • The registry entry has merged aliases naming causes and methods; should they be split off?