object

red dot galaxies

A type of compact, high-redshift galaxy appearing as red dots in observations.
80 related articles · 3 formulas

Description

Red dot galaxies are a class of compact, high-redshift galaxies that appear as small, red point-like sources in deep astronomical surveys. They were initially puzzling because their red colors suggested they might be dusty quasars, but observations with the James Webb Space Telescope revealed they are actually a new type of galaxy from the early Universe. These galaxies are extremely massive and form stars at a surprisingly high rate, yet they are so compact that their light is concentrated into a tiny angular size.

History

The term 'red dot galaxies' became prominent with the release of early James Webb Space Telescope data in 2022, which revealed these objects in unprecedented detail, challenging previous classifications.

How it works

The red color of these galaxies is not due to dust, but rather to their extreme distance: the expansion of the Universe stretches their light to longer, redder wavelengths (cosmological redshift). Their compactness means that the stars within them are packed tightly together, making them appear as point-like sources. The high star formation rates suggest they are undergoing intense bursts of star birth, possibly triggered by mergers or gas accretion in the early Universe.

In practice

These galaxies serve as probes of galaxy formation and evolution in the early Universe, helping astronomers understand how massive galaxies assembled within the first billion years after the Big Bang.

Fun fact

Some red dot galaxies appear to be so massive and so early in cosmic history that they initially seemed to challenge our standard model of cosmology, though later analysis showed they fit within it when accounting for measurement uncertainties.

Concept graph →

Formulas

$$(1+z_{\text{obs}}) = (1+z_1)(1+z_2)$$
Observed redshift is the product of component redshifts.
What is in the formula
z_obsvariableobserved total redshift — redshift
z_1variablefirst component redshift — redshift
z_2variablesecond component redshift — redshift
(1+z_{{obs}})=(1+z_\lambda)(1+z_q) · 2606.02097v1
$$z \approx \frac{v}{c}$$
Approximates cosmological redshift from radial velocity at low z.
What is in the formula
zvariableRedshift (fractional change in wavelength) — redshift
vvariableRadial velocity (recession speed) — velocity metre per second
cvariableSpeed of light in vacuum — speed of light metre per second
z\approx\frac{v}{c} · 2606.25022
$$1+z = \frac{\lambda_{\text{obs}}}{\lambda_{\text{em}}}}$$
Redshift defined as observed wavelength over emitted wavelength.
What is in the formula
zvariableredshift parameter — redshift
λ_obsvariableobserved wavelength — wavelength metre
λ_emvariableemitted wavelength — wavelength metre
1+z=\frac{λ_{obs}}{λ_{em}} · 2607.14525

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