About the Object

Exoplanet LHS 475 b (NIRSpec Transit Light Curve)

How do researchers spot a distant planet? By observing the changes in light as it orbits its star. A light curve from the NASA/ESA/CSA James Webb Space Telescope’s Near-Infrared Spectrograph (NIRSpec) shows the change in brightness from the LHS 475 star system over time as the planet transited the star on 31 August 2022. LHS 475 b is a rocky, Earth-sized exoplanet that orbits a red dwarf star roughly 41 light-years away, in the constellation Octans. The planet is extremely close to its star, completing one orbit in two Earth-days. Confirmation of the presence of the planet was made possible by Webb’s data.

[Image Description: The graphic shows the change in relative brightness of the star-planet system spanning three hours. The spectrum shows that the brightness of the system remains steady until the planet begins to transit the star. It then decreases, representing when the planet is directly in front of the star. The brightness increases again when the planet is no longer blocking the star, at which point it levels out.]


NASA, ESA, CSA, L. Hustak (STScI), K. Stevenson, J. Lustig-Yaeger, E. May (Johns Hopkins University Applied Physics Laboratory), G. Fu (Johns Hopkins University), and S. Moran (University of Arizona)

About the Image

Id: weic2302c
Type: Artwork
Release date: 11 January 2023, 19:15
Related releases: weic2302
Size: 15999 x 10479 px

Image Formats

Large JPEG 8.4 MB
Screensize JPEG 148.4 KB



1024x768 171.3 KB
1280x1024 252.5 KB
1600x1200 342.7 KB
1920x1200 411.8 KB
2048x1536 502.7 KB

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