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Atmospheric Remote-sensing Infrared Exoplanet Large-survey

future Mission
a diagram of the ARIEL satellite

The ARIEL mission from the European Space Agency (ESA) is a space telescope that can detect which atoms and molecules are present in the atmosphere of an exoplanet, looking to identify their temperatures and chemical processes. The mission will include a NASA instrument, CASE (the Contribution to ARIEL Spectroscopy of Exoplanets), which will observe clouds and hazes, and provide a more comprehensive picture of the exoplanet atmospheres ARIEL observes.

Type

Space Telescope

Launch

2028

Target

Universe

Objective

Explore the atmospheres of hundreds of exoplanets (planets orbiting stars beyond our Sun) for the first time
Learn more about Atmospheric Remote-sensing Infrared Exoplanet Large-survey
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James Webb Space Telescope

The image is divided horizontally by an undulating line between a cloudscape forming a nebula along the bottom portion and a comparatively clear upper portion. Speckled across both portions is a starfield, showing innumerable stars of many sizes. The smallest of these are small, distant, and faint points of light. The largest of these appear larger, closer, brighter, and more fully resolved with 8-point diffraction spikes. The upper portion of the image is blueish, and has wispy translucent cloud-like streaks rising from the nebula below. The orangish cloudy formation in the bottom half varies in density and ranges from translucent to opaque. The stars vary in color, the majority of which have a blue or orange hue. The cloud-like structure of the nebula contains ridges, peaks, and valleys – an appearance very similar to a mountain range. Three long diffraction spikes from the top right edge of the image suggest the presence of a large star just out of view.

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