File:NGC 3628 (noao-n3628saurdiff).jpg
Size of this preview: 605 × 600 pixels. Other resolutions: 242 × 240 pixels | 484 × 480 pixels | 775 × 768 pixels | 1,033 × 1,024 pixels | 1,935 × 1,918 pixels.
Original file (1,935 × 1,918 pixels, file size: 407 KB, MIME type: image/jpeg)
File information
Structured data
Captions
Summary edit
DescriptionNGC 3628 (noao-n3628saurdiff).jpg |
English: NGC 3628 is a remarkable galaxy since it is being disturbed in many ways. It is one member of a triple group of galaxies including M65 and M66 in Leo. The gravitational pull of these neighboring galaxies has most likely tipped the plane of NGC 3628 and made its central dust lane "wobbled" in appearance. In addition, spectroscopic analysis of the stars and gas in the disk reveal interesting kinematics. The stars orbit the galaxy in the opposite direction of the gas. It is surmised that a recent galactic mergers generates these kinds of dynamics. In this image, there are many small galaxies (especially the dim dwarf beneath) which may soon be gobbled up. All of this action takes place some 35 million light years away from us.This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
Date | 27 March 2014, 14:05:00 (upload date) |
Source | NGC 3628 |
Author | KPNO/NOIRLab/NSF/AURA/Glen Saurdiff and Joan Simpson/F. Haase, S. Peterson, K. Garmany |
Other versions |
|
Licensing edit
This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week 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 | 17:46, 23 October 2023 | 1,935 × 1,918 (407 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/noao-n3628saurdiff.jpg via Commons:Spacemedia |
You cannot overwrite this file.
File usage on Commons
The following page uses 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 |
|
---|---|
Credit/Provider | KPNO/NOIRLab/NSF/AURA/Glen Saurdiff and Joan Simpson/F. Haase, S. Peterson, K. Garmany |
Source | NSF's NOIRLab |
Short title |
|
Usage terms |
|
Date and time of data generation | 14:05, 27 March 2014 |
JPEG file comment | NGC 3628 is a remarkable galaxy since it is being disturbed in many ways. It is one member of a triple group of galaxies including M65 and M66 in Leo. The gravitational pull of these neighboring galaxies has most likely tipped the plane of NGC 3628 and made its central dust lane "wobbled" in appearance. In addition, spectroscopic analysis of the stars and gas in the disk reveal interesting kinematics. The stars orbit the galaxy in the opposite direction of the gas. It is surmised that a recent galactic mergers generates these kinds of dynamics. In this image, there are many small galaxies (especially the dim dwarf beneath) which may soon be gobbled up. All of this action takes place some 35 million light years away from us. This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 16:07, 15 September 2021 |
Unique ID of original document | uuid:935AF79C9F88E0119CDEE6B0DAB1BB4F |
Date and time of digitizing | 06:28, 27 May 2011 |
Date metadata was last modified | 11:07, 15 September 2021 |
Keywords | NGC 3628 |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |