About the Object

Name:	NGC 4449
Distance:	12 million light years
Constellation:	Canes Venatici
Category:	Galaxies MIRI Picture of the Month

Coordinates

Position (RA):	12 28 10.71
Position (Dec):	44° 5' 43.40"
Field of view:	3.58 x 2.07 arcminutes
Orientation:	North is 137.0° right of vertical

View in ESASky:

View in WorldWide Telescope:

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Optical (DSS2)
Infrared (2MASS)

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Colours & filters

Band	Wavelength	Telescope
Infrared	5.6 μm	James Webb Space Telescope MIRI
Infrared	5.6 μm	James Webb Space Telescope MIRI
Infrared PAH	7.7 μm	James Webb Space Telescope MIRI
Infrared PAH	7.7 μm	James Webb Space Telescope MIRI

NGC 4449 (MIRI)

Featured in this new image from the NASA/ESA/CSA James Webb Space Telescope is the dwarf galaxy NGC 4449. This galaxy, also known as Caldwell 21, resides roughly 12.5 million light-years away in the constellation Canes Venatici. It is part of the M94 galaxy group, which lies close to the Local Group that hosts our Milky Way.

NGC 4449 has been forming stars for several billion years, but it is currently experiencing a period of star formation at a much higher rate than in the past. Such unusually explosive and intense star formation activity is called a starburst and for that reason NGC 4449 is known as a starburst galaxy. In fact, at the current rate of star formation, the gas supply that feeds the production of stars would only last for another billion years or so. Starbursts usually occur in the central regions of galaxies, but NGC 4449 displays more widespread star formation activity, and the very youngest stars are observed both in the nucleus and in streams surrounding the galaxy. It's likely that the current widespread starburst was triggered by interaction or merging with a smaller companion; indeed, astronomers think NGC 4449's star formation has been influenced by interactions with several of its neighbours.

NGC 4449 resembles primordial star-forming galaxies which grew by merging with and accreting smaller stellar systems. Since NGC 4449 is close enough to be observed in great detail, it is the ideal laboratory for astronomers to study what may have occurred during galaxy formation and evolution in the early Universe.

This image was captured with Webb’s MIRI, or the Mid-InfraRed Instrument, makes observations in the mid-infrared, which spans wavelengths of light very different from visible light the wavelengths that human eyes are sensitive to, which extend from about 0.38 to 0.75 micrometres (a micrometre, or micron, is one thousandth of a millimetre). By contrast, MIRI detects light between 5 and 28 micrometres. However, it does not typically observe across this entire wavelength range all at once. Instead, MIRI has a set of ten filters that allow very specific regions of light through. For example, one of MIRI’s filters used in this image (named F770W), allows light with wavelengths from 6.581 to 8.687 micrometres to pass through it.

This MIRI image reveals the galaxy’s creeping tendrils of gas, dust and stars. The bright blue spots reveal countless individual stars, while the bright yellow regions that weave throughout the galaxy indicate concentrations of active stellar nurseries, where new stars are forming. The orange-red areas indicate the distribution of a type of carbon-based compounds known as polycyclic aromatic hydrocarbons (or PAHs) — the F770W filter is particularly suited to imaging these important molecules.

[Image Description: A close-in view of the central area of a dwarf galaxy. Large, smoky clouds of gas and dust billow out across the scene. They are portrayed in warm colours which indicate the composition of the dust: brightest in the centre, and darker out to the galaxy’s edge. Its core — a large, bright dot in the centre — and many pointlike stars shine through gaps in the dust, as do some small, distant galaxies in the background.]