File:Comet Hyakutake (eso9610a).tiff
Original file (1,070 × 531 pixels, file size: 653 KB, MIME type: image/tiff)
Captions
Summary
[edit]DescriptionComet Hyakutake (eso9610a).tiff |
English: These false-colour photos show the first images of comet C/1996 B2 (Hyakutake), obtained with the DFOSC instrument at the Danish 1.54-metre telescope at the ESO La Silla Observatory. This comet is expected to become quite bright when it passes near the Earth in late March 1996. The observations were made by Jean-Marie Will, visiting astronomer from Sternwarte der Universitaet Bonn, Germany. The images have been reproduced from two CCD frames with 6 and 20 min exposure time, respectively. They were obtained through a standard V-filter just after 08:00 UT on 9 February 1996. The instrument was DFOSC with the Danish Loral/Lesser CCD (2052 x 2052 pix; 0.39 arcsec/pix; field of view 13.3 x 13.3 arcmin). For this presentation, the original CCD frames were bias-subtracted, flat-fielded, cleaned and the field was trimmed to 10.4 x 10.4 arcmin. North is up and East is to the left. The cometary coma which consists of dust and gas emitted by the nucleus is elongated in the anti-solar direction (p.a. = 289 deg; counted from North over East); the tear-shaped form is indicative of the beginning development of a dust tail. Otherwise, the coma is very symmetrical and there is no evidence of any jets or outflows. The largest diameter on the 20-min exposure is about 7 arcmin. At the time of this observation, the comet was at a distance of 1.52 AU (227 million kilometres) from the Earth and 1.88 AU (281 million kilometres) from the Sun. |
||
Date | 11 February 1996 (upload date) | ||
Source |
|
||
Author | ESO | ||
Other versions |
|
Licensing
[edit]This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:36, 16 June 2024 | 1,070 × 531 (653 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://www.eso.org/public/archives/images/original/eso9610a.tif via Commons:Spacemedia |
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 | These false-colour photos show the first images of comet C/1996 B2 (Hyakutake), obtained with the DFOSC instrument at the Danish 1.54-metre telescope at the ESO La Silla Observatory. This comet is expected to become quite bright when it passes near the Earth in late March 1996. The observations were made by Jean-Marie Will, visiting astronomer from Sternwarte der Universitaet Bonn, Germany. The images have been reproduced from two CCD frames with 6 and 20 min exposure time, respectively. They were obtained through a standard V-filter just after 08:00 UT on 9 February 1996. The instrument was DFOSC with the Danish Loral/Lesser CCD (2052 x 2052 pix; 0.39 arcsec/pix; field of view 13.3 x 13.3 arcmin). For this presentation, the original CCD frames were bias-subtracted, flat-fielded, cleaned and the field was trimmed to 10.4 x 10.4 arcmin. North is up and East is to the left. The cometary coma which consists of dust and gas emitted by the nucleus is elongated in the anti-solar direction (p.a. = 289 deg; counted from North over East); the tear-shaped form is indicative of the beginning development of a dust tail. Otherwise, the coma is very symmetrical and there is no evidence of any jets or outflows. The largest diameter on the 20-min exposure is about 7 arcmin. At the time of this observation, the comet was at a distance of 1.52 AU (227 million kilometres) from the Earth and 1.88 AU (281 million kilometres) from the Sun. |
---|---|
Width | 1,070 px |
Height | 531 px |
Bits per component |
|
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 81 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CC 2015 (Macintosh) |
File change date and time | 14:43, 19 July 2016 |
Color space | sRGB |