File:TRAPPIST-1 c Light Curve.jpg

Page contents not supported in other languages.
This is a file from the Wikimedia Commons
From Wikipedia, the free encyclopedia

Original file(3,840 × 2,160 pixels, file size: 594 KB, MIME type: image/jpeg)

Summary

Description
English: This light curve shows the change in brightness of the TRAPPIST-1 system as the second planet, TRAPPIST-1 c, moves behind the star. This phenomenon is known as a secondary eclipse.

Astronomers used Webb’s Mid-Infrared Instrument (MIRI) to measure the brightness of mid-infrared light. When the planet is beside the star, the light emitted by both the star and the dayside of the planet reach the telescope, and the system appears brighter. When the planet is behind the star, the light emitted by the planet is blocked and only the starlight reaches the telescope, causing the apparent brightness to decrease.

Astronomers can subtract the brightness of the star from the combined brightness of the star and planet to calculate how much infrared light is coming from the planet’s dayside. This is then used to calculate the dayside temperature and infer the presence and possible composition of the atmosphere.

The graph shows combined data from four separate observations made using MIRI’s F1500W filter, which only allows light with wavelengths ranging from about 13.5 - 16.7 microns to pass through to the detectors. The blue squares are individual brightness measurements. The red circles show measurements that are “binned,” or averaged to make it easier to see the change over time. The white line is the best fit, or model light curve that matches the data most closely. The decrease in brightness during the secondary eclipse is less than 0.05%.

The temperature calculated from this observation is 380 +/- 31 kelvins (between 170 and 280 degrees Fahrenheit). TRAPPIST-1 c is the coolest rocky exoplanet ever observed using secondary eclipse photometry.
Date
Source https://webbtelescope.org/contents/media/images/2023/125/01H2TM6BH195YDAAWQ29BAFW38
Author NASA, ESA, CSA, Joseph Olmsted (STScI)

Licensing

Public domain This file is in the public domain because it was created by NASA, ESA and CSA. NASA Webb material is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA/CSA is credited as the source of the material. This license does not apply if source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-03127. Copyright statement at webbtelescope.org.
For material created by the European Space Agency on the esawebb.org site, use the {{ESA-Webb}} tag.

Captions

Secondary eclipse light curve of TRAPPIST-1 c

Items portrayed in this file

depicts

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current17:19, 19 June 2023Thumbnail for version as of 17:19, 19 June 20233,840 × 2,160 (594 KB)SevenSpheresUploaded a work by NASA, ESA, CSA, Joseph Olmsted (STScI) from https://webbtelescope.org/contents/media/images/2023/125/01H2TM6BH195YDAAWQ29BAFW38 with UploadWizard
The following pages on the English Wikipedia use this file (pages on other projects are not listed):

Metadata