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DescriptionComposition of cloud particles - hot gas giant exoplanet WASP-17b (WASP17b).jpg |
English: This is a
transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by Webb’s Mid-Infrared Instrument (
MIRI) on 12-13 March 2023. It reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet.This marks the first time that SiO2 has been identified in an exoplanet, and the first time any specific cloud species has been identified in a transiting exoplanet.The spectrum was made by measuring the change in brightness of 28 wavelength-bands of mid-infrared light as the planet transited the star. Webb observed the WASP-17 system using MIRI’s low-resolution spectrograph for nearly 10 hours, collecting more than 1,275 measurements before, during, and after the transit.For each wavelength, the amount of light blocked by the planet’s atmosphere (white circles) was calculated by subtracting the amount that made it through the atmosphere from the amount originally emitted by the star.The solid purple line is a best-fit model to the Webb (MIRI), Hubble, and Spitzer data (the Hubble and Spitzer data cover wavelengths from 0.34 to 4.5 microns and are not shown on the graph). The spectrum shows a clear feature around 8.6 microns, which astronomers think is caused by silica particles absorbing some of the starlight passing through the atmosphere.The dashed yellow line shows what that part of the transmission spectrum would look like if the clouds in WASP-17 b’s atmosphere did not contain SiO2. |
Date | 16 October 2023 (upload date) |
Source | Composition of cloud particles - hot gas giant exoplanet WASP-17b |
Author | NASA, ESA, CSA, R. Crawford (STScI), D. Grant (University of Bristol), H. R. Wakeford (University of Bristol), N. Lewis (Cornell University) |
Other versions |
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ESA/Webb images, videos and web texts are released by the
ESA under the
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current | 10:00, 17 October 2023 | 3,840 × 2,455 (727 KB) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esawebb.org/archives/images/large/WASP17b.jpg via Commons:Spacemedia |
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Source | ESA/Webb |
---|---|
Credit/Provider | NASA, ESA, CSA, R. Crawford (STScI), D. Grant (University of Bristol), H. R. Wakeford (University of Bristol), N. Lewis (Cornell University) |
Usage terms |
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Short title |
|
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Date and time of data generation | 16:00, 16 October 2023 |
JPEG file comment | This is a transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by Webb’s Mid-Infrared Instrument (MIRI) on 12-13 March 2023. It reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet. This marks the first time that SiO2 has been identified in an exoplanet, and the first time any specific cloud species has been identified in a transiting exoplanet. The spectrum was made by measuring the change in brightness of 28 wavelength-bands of mid-infrared light as the planet transited the star. Webb observed the WASP-17 system using MIRI’s low-resolution spectrograph for nearly 10 hours, collecting more than 1,275 measurements before, during, and after the transit. For each wavelength, the amount of light blocked by the planet’s atmosphere (white circles) was calculated by subtracting the amount that made it through the atmosphere from the amount originally emitted by the star. The solid purple line is a best-fit model to the Webb (MIRI), Hubble, and Spitzer data (the Hubble and Spitzer data cover wavelengths from 0.34 to 4.5 microns and are not shown on the graph). The spectrum shows a clear feature around 8.6 microns, which astronomers think is caused by silica particles absorbing some of the starlight passing through the atmosphere. The dashed yellow line shows what that part of the transmission spectrum would look like if the clouds in WASP-17 b’s atmosphere did not contain SiO2. |
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
Original file (3,840 × 2,455 pixels, file size: 727 KB, MIME type: image/jpeg)
This is a file from the
Wikimedia Commons. Information from its
description page there is shown below. Commons is a freely licensed media file repository. You can help. |
DescriptionComposition of cloud particles - hot gas giant exoplanet WASP-17b (WASP17b).jpg |
English: This is a
transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by Webb’s Mid-Infrared Instrument (
MIRI) on 12-13 March 2023. It reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet.This marks the first time that SiO2 has been identified in an exoplanet, and the first time any specific cloud species has been identified in a transiting exoplanet.The spectrum was made by measuring the change in brightness of 28 wavelength-bands of mid-infrared light as the planet transited the star. Webb observed the WASP-17 system using MIRI’s low-resolution spectrograph for nearly 10 hours, collecting more than 1,275 measurements before, during, and after the transit.For each wavelength, the amount of light blocked by the planet’s atmosphere (white circles) was calculated by subtracting the amount that made it through the atmosphere from the amount originally emitted by the star.The solid purple line is a best-fit model to the Webb (MIRI), Hubble, and Spitzer data (the Hubble and Spitzer data cover wavelengths from 0.34 to 4.5 microns and are not shown on the graph). The spectrum shows a clear feature around 8.6 microns, which astronomers think is caused by silica particles absorbing some of the starlight passing through the atmosphere.The dashed yellow line shows what that part of the transmission spectrum would look like if the clouds in WASP-17 b’s atmosphere did not contain SiO2. |
Date | 16 October 2023 (upload date) |
Source | Composition of cloud particles - hot gas giant exoplanet WASP-17b |
Author | NASA, ESA, CSA, R. Crawford (STScI), D. Grant (University of Bristol), H. R. Wakeford (University of Bristol), N. Lewis (Cornell University) |
Other versions |
|
ESA/Webb images, videos and web texts are released by the
ESA under the
Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the
ESA copyright statement for full information. For images created by NASA or on the webbtelescope.org website, use the
{{PD-Webb}} tag.
Conditions:
Notes:
|
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 10:00, 17 October 2023 | 3,840 × 2,455 (727 KB) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esawebb.org/archives/images/large/WASP17b.jpg via Commons:Spacemedia |
The following other wikis use this file:
This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
If the file has been modified from its original state, some details may not fully reflect the modified file.
Source | ESA/Webb |
---|---|
Credit/Provider | NASA, ESA, CSA, R. Crawford (STScI), D. Grant (University of Bristol), H. R. Wakeford (University of Bristol), N. Lewis (Cornell University) |
Usage terms |
|
Short title |
|
Image title |
|
Date and time of data generation | 16:00, 16 October 2023 |
JPEG file comment | This is a transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by Webb’s Mid-Infrared Instrument (MIRI) on 12-13 March 2023. It reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet. This marks the first time that SiO2 has been identified in an exoplanet, and the first time any specific cloud species has been identified in a transiting exoplanet. The spectrum was made by measuring the change in brightness of 28 wavelength-bands of mid-infrared light as the planet transited the star. Webb observed the WASP-17 system using MIRI’s low-resolution spectrograph for nearly 10 hours, collecting more than 1,275 measurements before, during, and after the transit. For each wavelength, the amount of light blocked by the planet’s atmosphere (white circles) was calculated by subtracting the amount that made it through the atmosphere from the amount originally emitted by the star. The solid purple line is a best-fit model to the Webb (MIRI), Hubble, and Spitzer data (the Hubble and Spitzer data cover wavelengths from 0.34 to 4.5 microns and are not shown on the graph). The spectrum shows a clear feature around 8.6 microns, which astronomers think is caused by silica particles absorbing some of the starlight passing through the atmosphere. The dashed yellow line shows what that part of the transmission spectrum would look like if the clouds in WASP-17 b’s atmosphere did not contain SiO2. |
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |