Αρχείο:Boulevard of Broken Rings.jpg
Εικόνα σε υψηλότερη ανάλυση (2.659 × 1.461 εικονοστοιχεία, μέγεθος αρχείου: 791 KB, τύπος MIME: image/jpeg)
Αυτό το αρχείο και η περιγραφή του προέρχονται από το Wikimedia Commons. Οι πληροφορίες από την σελίδα περιγραφής του εκεί εμφανίζονται παρακάτω. |
Σύνοψη
ΠεριγραφήBoulevard of Broken Rings.jpg |
English: This Picture of the Week illustrates the remarkable capabilities of SPHERE (the Spectro-Polarimetric High-contrast Exoplanet REsearch instrument), a planet-hunting instrument mounted on ESO’s Very Large Telescope (VLT) in Chile: It shows a series of broken rings of dust around a nearby star. These concentric rings are located in the inner region of the debris disc surrounding a young star named HD 141569A, which sits some 370 light-years away from us.
In this image we see what is known as a transition disc, a short-lived stage between the protoplanetary phase, when planets have not yet formed, and a later time when planets have coalesced, leaving the disc populated only by any remaining — and predominantly dusty — debris. What we see here are structures formed of dust, revealed for the first time in near-infrared light by SPHERE — at a high enough resolution to capture remarkable detail! The area shown in this image has a diameter of just 200 times the Earth–Sun distance. Several features are visible, including a bright, prominent ring with well-defined edges — so asymmetric that it appears as a half-ring — multiple clumps, several concentric ringlets, and a pattern akin to a spiral arm. It is significant that these structures are asymmetric; this may reflect an uneven, or clumpy, distribution of dust in the disc, something for which astronomers do not currently have a firm explanation. It is possible that this phenomenon is caused by the presence of planets, but so far no planets of sufficient size to do this have been found in this system. |
Ημερομηνία | |
Πηγή | http://www.eso.org/public/images/potw1625a/ |
Δημιουργός | ESO/Perrot |
Αδειοδότηση
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. | |
Το αρχείο διανέμεται υπό την άδεια Creative Commons Αναφορά προέλευσης 4.0 Διεθνής
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Items portrayed in this file
απεικονίζει
20 Ιουνίου 2016
image/jpeg
checksum Αγγλικά
6b4f7fed1fdada92854379703a3db828b44af4ea
data size Αγγλικά
147.082 Byte
703 εικονοστοιχείο
1.280 εικονοστοιχείο
Ιστορικό αρχείου
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Ώρα/Ημερομ. | Μικρογραφία | Διαστάσεις | Χρήστης | Σχόλια | |
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τελευταία | 11:44, 14 Φεβρουαρίου 2024 | 2.659 × 1.461 (791 KB) | C messier | full size | |
11:02, 21 Ιουνίου 2016 | 1.280 × 703 (144 KB) | Jmencisom | User created page with UploadWizard |
Συνδέσεις αρχείου
Τα παρακάτω λήμματα συνδέουν σε αυτό το αρχείο:
Καθολική χρήση αρχείου
Τα ακόλουθα άλλα wiki χρησιμοποιούν αυτό το αρχείο:
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Μεταδεδομένα
Αυτό το αρχείο περιέχει πρόσθετες πληροφορίες, πιθανόν από την ψηφιακή φωτογραφική μηχανή ή το scanner που χρησιμοποιήθηκε για την δημιουργία ή την ψηφιοποίησή της. Αν το αρχείο έχει τροποποιηθεί από την αρχική του κατάσταση, ορισμένες λεπτομέρειες πιθανόν να μην αντιστοιχούν πλήρως στην τροποποιημένη εικόνα.
Αναφορά/Πάροχος | ESO/Perrot |
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Πηγή | European Southern Observatory |
Συνοπτικός τίτλος |
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Τίτλος εικόνας |
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Όροι χρήσης |
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Ημερομηνία και ώρα της παραγωγής ψηφιακών δεδομένων | 06:00, 20 Ιουνίου 2016 |
Σχόλιο αρχείου JPEG | This Picture of the Week illustrates the remarkable capabilities of SPHERE (the Spectro-Polarimetric High-contrast Exoplanet REsearch instrument), a planet-hunting instrument mounted on ESO’s Very Large Telescope (VLT) in Chile: It shows a series of broken rings of dust around a nearby star. These concentric rings are located in the inner region of the debris disc surrounding a young star named HD 141569A, which sits some 370 light-years away from us. In this image we see what is known as a transition disc, a short-lived stage between the protoplanetary phase, when planets have not yet formed, and a later time when planets have coalesced, leaving the disc populated only by any remaining — and predominantly dusty — debris. What we see here are structures formed of dust, revealed for the first time in near-infrared light by SPHERE — at a high enough resolution to capture remarkable detail! The area shown in this image has a diameter of just 200 times the Earth–Sun distance. Several features are visible, including a bright, prominent ring with well-defined edges — so asymmetric that it appears as a half-ring — multiple clumps, several concentric ringlets, and a pattern akin to a spiral arm. It is significant that these structures are asymmetric; this may reflect an uneven, or clumpy, distribution of dust in the disc, something for which astronomers do not currently have a firm explanation. It is possible that this phenomenon is caused by the presence of planets, but so far no planets of sufficient size to do this have been found in this system. Links: Research paper — C. Perrot et al., Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE. |
Λέξεις κλειδιά | HD 141569 |
Στοιχεία επικοινωνίας |
Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
Έκδοση IIM | 4 |