File:NGC 1022.png

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Original file(2,038 × 1,919 pixels, file size: 19 MB, MIME type: image/png)

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Description

This is a new view of the central region of the interesting NGC 1022, classified as a compact barred spiral galaxy. There isn't that much dust or star formation in this one and it seems to be boarding on being a lenticular galaxy. Hubble looked at this galaxy many years ago, with the WFPC2 instrument, so I instantly recognised this galaxy when I saw it on the archive. To say I got excited would be an understatement. Seeing familiar things in an amazingly higher resolution is always nice.

The core appears to be super colourful and vibrant, so I wonder if there's more going on in this galaxy than meets the eye. It still seems very old. There are lots of globular clusters, something I never noticed with the WFPC2 data. This proposal is just fantastic and I'm completely raiding it.

Morphological type: SBa

Red: WFC3/IR F160W Green: WFC3/UVIS F814W

Blue: WFC3/UVIS F475W
Date
Source NGC 1022
Author solomon from USA

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This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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This image was originally posted to Flickr by theantarcticsun at https://flickr.com/photos/131716393@N07/32039590228 (archive). It was reviewed on 28 September 2019 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

28 September 2019

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Date/TimeThumbnailDimensionsUserComment
current09:05, 28 September 2019Thumbnail for version as of 09:05, 28 September 20192,038 × 1,919 (19 MB)Fabian RRRR (talk | contribs)=={{int:filedesc}}== {{Information |Description=This is a new view of the central region of the interesting NGC 1022, classified as a compact barred spiral galaxy. There isn't that much dust or star formation in this one and it seems to be boarding on being a lenticular galaxy. Hubble looked at this galaxy many years ago, with the WFPC2 instrument, so I instantly recognised this galaxy when I saw it on the archive. To say I got excited would be an understatement. Seeing familiar things in an...

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