File:Artist’s impression of the dwarf planet Eris and its moon Dysnomia.tif
![File:Artist’s impression of the dwarf planet Eris and its moon Dysnomia.tif](https://upload.wikimedia.org/wikipedia/commons/thumb/b/bd/Artist%E2%80%99s_impression_of_the_dwarf_planet_Eris_and_its_moon_Dysnomia.tif/lossy-page1-800px-Artist%E2%80%99s_impression_of_the_dwarf_planet_Eris_and_its_moon_Dysnomia.tif.jpg?20231203183035)
Size of this JPG preview of this TIF file: 800 × 533 pixels. Other resolutions: 320 × 213 pixels | 640 × 427 pixels | 1,024 × 683 pixels | 1,280 × 853 pixels | 2,560 × 1,707 pixels | 4,500 × 3,000 pixels.
Original file (4,500 × 3,000 pixels, file size: 24.31 MB, MIME type: image/tiff)
File information
Structured data
Captions
Captions
Add a one-line explanation of what this file represents
Summary
editDescriptionArtist’s impression of the dwarf planet Eris and its moon Dysnomia.tif | This artist's impression shows the distant dwarf planet Eris in the distance with its moon Dysmonia in the foreground. New observations have shown that Eris is smaller than previously thought and almost exactly the same size as Pluto. Eris is extremely reflective and its surface is probably covered in frost formed from the frozen remains of its atmosphere. Dysnomia appears to be a darker and less reflective body. | ||||
Date | 26 October 2011, 19:00 | ||||
Source | https://www.eso.org/public/images/eso1142c/ | ||||
Author | ESO/L. Calçada and Nick Risinger | ||||
Permission (Reusing this file) |
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 18:30, 3 December 2023 | ![]() | 4,500 × 3,000 (24.31 MB) | Юрий Д.К. (talk | contribs) | {{Information |Description=This artist's impression shows the distant dwarf planet Eris in the distance with its moon Dysmonia in the foreground. New observations have shown that Eris is smaller than previously thought and almost exactly the same size as Pluto. Eris is extremely reflective and its surface is probably covered in frost formed from the frozen remains of its atmosphere. Dysnomia appears to be a darker and less reflective body. |Source=https://www.eso.org/public/images/eso1142c/ |... |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title | This artist's impression shows the distant dwarf planet Eris in the distance with its moon Dysmonia in the foreground. New observations have shown that Eris is smaller than previously thought and almost exactly the same size as Pluto. Eris is extremely reflective and its surface is probably covered in frost formed from the frozen remains of its atmosphere. Dysnomia appears to be a darker and less reflective body. |
---|---|
Width | 4,500 px |
Height | 3,000 px |
Bits per component |
|
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 19 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS5 Macintosh |
File change date and time | 12:20, 25 October 2011 |
Color space | Uncalibrated |