File:Galactic Conjunction - Flickr - NASA Hubble.jpg
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Summary
editDescriptionGalactic Conjunction - Flickr - NASA Hubble.jpg |
This spectacular image from the Hubble Space Telescope captures the spiral galaxy NGC 105, which lies roughly 215 million light-years away in the constellation Pisces. While it looks like NGC 105 is plunging edge-on into a neighboring galaxy, this is just a circumstance of perspective. NGC 105’s elongated neighbor is actually far more distant. Such visual associations are the result of our Earthly perspective and they occur frequently in astronomy. Hubble’s Wide Field Camera 3 observations in this image are from a vast collection of Hubble measurements examining nearby galaxies that contain two fascinating astronomical phenomena – Cepheid variable stars and cataclysmic supernova explosions. While these two phenomena may appear unrelated – one is a peculiar class of pulsating stars and the other is the explosion caused by the catastrophic death of a massive star – astronomers use both to measure the vast distances to astronomical objects. Both Cepheids and supernovae have very predictable luminosities. Astronomers use these so-called “standard candles” to determine distances by comparing how bright these objects appear from Earth to their actual brightness. NGC 105 contains both supernovae and Cepheid variables, giving astronomers the opportunity to calibrate the two distance measurement techniques against one another. Credit: ESA/Hubble & NASA, D. Jones, A. Riess et al. Acknowledgement: R. Colombari For more information, visit: esahubble.org/images/potw2201a/ Find us on Twitter, Instagram, Facebook and YouTube |
Date | Taken on 3 January 2022, 06:00 |
Source | Galactic Conjunction |
Author | NASA Hubble Space Telescope |
Flickr tags InfoField | ngc 105 , nasa , hubble , esa , hubble space telescope , telescope , space telescope , cosmos , universe , space , cosmic , astronomy , galaxy , galaxies , spiral galaxy |
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This image was originally posted to Flickr by NASA Hubble at https://flickr.com/photos/144614754@N02/52046618510. It was reviewed on 7 May 2022 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
7 May 2022
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current | 07:11, 7 May 2022 | 3,565 × 2,045 (5.75 MB) | Red panda bot (talk | contribs) | In Flickr Explore: 2022-05-03 |
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Date and time of data generation | 06:00, 3 January 2022 |
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Short title | Galactic Conjunction |
Credit/Provider | ESA/Hubble & NASA, D. Jones, A. |
Source | ESA/Hubble |
Image title | This image from the NASA/ESA Hubble Space Telescope captures the spiral galaxy NGC 105, which lies roughly 215 million light-years away in the constellation Pisces. While it looks like NGC 105 is plunging edge-on into a collision with a neighbouring galaxy, this is just the result of the chance alignment of the two objects in the night sky. NGC 105’s elongated neighbour is actually far more distant and remains relatively unknown to astronomers. These misleading conjunctions occur frequently in astronomy — for example, the stars in constellations are at vastly different distances from Earth, and only appear to form patterns thanks to the chance alignment of their component stars. The Wide Field Camera 3 observations in this image are from a vast collection of Hubble measurements examining nearby galaxies which contain two fascinating astronomical phenomena — Cepheid variables and cataclysmic supernova explosions. Whilst these two phenomena may appear to be unrelated — one is a peculiar class of pulsating stars and the other is the explosion caused by the catastrophic final throes of a massive star’s life — they are both used by astronomers for a very particular purpose: measuring the vast distances to astronomical objects. Both Cepheids and supernovae have very predictable luminosities, meaning that astronomers can tell precisely how bright they are. By measuring how bright they appear when observed from Earth, these “standard candles” can provide reliable distance measurements. NGC 105 contains both supernovae and Cepheid variables, giving astronomers a valuable opportunity to calibrate the two distance measurement techniques against one another. Astronomers recently carefully analysed the distances to a sample of galaxies including NGC 105 to measure how fast the Universe is expanding — a value known as the Hubble constant. Their results don’t agree with the predictions of the most widely-accepted cosmological model, and their analysis shows tha |
Publisher | ESA/Hubble |
Usage terms |
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JPEG file comment | This image from the NASA/ESA Hubble Space Telescope captures the spiral galaxy NGC 105, which lies roughly 215 million light-years away in the constellation Pisces. While it looks like NGC 105 is plunging edge-on into a collision with a neighbouring galaxy, this is just the result of the chance alignment of the two objects in the night sky. NGC 105’s elongated neighbour is actually far more distant and remains relatively unknown to astronomers. These misleading conjunctions occur frequently in astronomy — for example, the stars in constellations are at vastly different distances from Earth, and only appear to form patterns thanks to the chance alignment of their component stars. The Wide Field Camera 3 observations in this image are from a vast collection of Hubble measurements examining nearby galaxies which contain two fascinating astronomical phenomena — Cepheid variables and cataclysmic supernova explosions. Whilst these two phenomena may appear to be unrelated — one is a peculiar class of pulsating stars and the other is the explosion caused by the catastrophic final throes of a massive star’s life — they are both used by astronomers for a very particular purpose: measuring the vast distances to astronomical objects. Both Cepheids and supernovae have very predictable luminosities, meaning that astronomers can tell precisely how bright they are. By measuring how bright they appear when observed from Earth, these “standard candles” can provide reliable distance measurements. NGC 105 contains both supernovae and Cepheid variables, giving astronomers a valuable opportunity to calibrate the two distance measurement techniques against one another. Astronomers recently carefully analysed the distances to a sample of galaxies including NGC 105 to measure how fast the Universe is expanding — a value known as the Hubble constant. Their results don’t agree with the predictions of the most widely-accepted cosmological model, and their analysis shows that there is only a 1-in-a-million chance that this discrepancy was caused by measurement errors. This discrepancy between galaxy measurements and cosmological predictions has been a long-standing source of consternation for astronomers, and these recent findings provide persuasive new evidence that something is either wrong or lacking in our standard model of cosmology. |
Orientation | Normal |
Horizontal resolution | 25.4 dpi |
Vertical resolution | 25.4 dpi |
Software used | Adobe Photoshop 23.0 (Windows) |
File change date and time | 00:10, 17 December 2021 |
Y and C positioning | Centered |
Exif version | 2.32 |
Date and time of digitizing | 11:58, 1 December 2021 |
Meaning of each component |
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Supported Flashpix version | 1 |
Color space | Uncalibrated |
IIM version | 4 |
Keywords | NGC 105 |
Bits per component |
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Compression scheme | Uncompressed |
Height | 2,045 px |
Width | 3,565 px |
Pixel composition | RGB |
Number of components | 3 |
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
Type of media | Observation |
Date metadata was last modified | 01:10, 17 December 2021 |
Unique ID of original document | xmp.did:9a1623c7-0e85-7548-af14-af4ae657b2aa |