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Summary

DescriptionNASA-EarlyEarth-PaleOrangeDot-20190802.jpg
English: When haze built up in the——atmosphere of Archean Earth, "the young planet might have looked like this artist's interpretation - a pale orange dot." A team led by, Goddard scientists thinks the "haze was self-limiting," cooling the surface by about 36 degrees Fahrenheit (20 Kelvins) – not enough——to cause runaway glaciation. The team’s modeling suggests that atmospheric haze might be, "helpful for identifying earthlike exoplanets that could be habitable."
Date
Source https://www.flickr.com/photos/gsfc/32407459560; see also https://www.nasa.gov/feature/goddard/2019/shining-starlight-on-the-search-for-life and https://www.nasa.gov/feature/goddard/2017/nasa-team-looks-to-ancient-earth-first-to-study-hazy-exoplanets
Author NASA/Goddard Space Flight Center/Francis Reddy

Licensing

Public domainPublic domainfalsefalse
Public domain This file is in the public domain in the United States. Because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page/JPL Image Use Policy.)
Warnings:

Captions

NASA - Early Earth - Pale Orange Dot - August 2, 2019

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depicts

1 February 2017

image/jpeg

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Date/TimeThumbnailDimensionsUserComment
current01:09, 6 August 2019Thumbnail for version as of 01:09, 6 August 20193,840 × 2,160 (1.71 MB)HuntsterHigher resolution version.
17:54, 3 August 2019Thumbnail for version as of 17:54, 3 August 20191,440 × 810 (72 KB)DrbogdanUser created page with UploadWizard

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Width3,840 px
Height2,160 px
Bits per component
  • 8
  • 8
  • 8
Pixel compositionRGB
OrientationNormal
Number of components3
Horizontal resolution300 dpi
Vertical resolution300 dpi
Software usedAdobe Photoshop CC 2015 (Windows)
File change date and time01:01, 2 February 2017
Exif version2.21
Color spaceUncalibrated
Date and time of digitizing21:43, 31 January 2017
Date metadata was last modified20:01, 1 February 2017
Unique ID of original documentxmp.did:c3cf5860-f131-4a43-b8a9-d3c84d03932a
IIM version24,832

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