Fasciculus:Swift j1818 inset.jpg

Sua resolutio ‎(864 × 864 elementa imaginalia, magnitudo fasciculi: 321 chiliocteti, typus MIME: image/jpeg)

Hic fasciculus apud Vicimedia Communia iacet; in aliis inceptis adhiberi potest. Contenta paginae descriptionis fasciculi subter monstrantur.

Summarium

DescriptioSwift j1818 inset.jpg	English: This image contains an exceptional magnetar, a type of neutron star with very powerful magnetic fields. Astronomers have found evidence that this object may be the youngest known magnetar (about 500 years old in Earth's timeframe). It is also the fastest rotating one yet discovered (spinning about 1.4 times per second). This image shows the magnetar in X-rays from Chandra (purple) at the center of the image in combination with Spitzer and WISE infrared data showing the wider field of view. Magnetars form when a massive star runs out of nuclear fuel and its core collapses onto itself.
Datum	8 Ianuarius 2021
Fons	https://chandra.harvard.edu/photo/2021/j1818/
Auctor	X-ray: NASA/CXC/Univ. of West Virginia/H. Blumer; Infrared (Spitzer and Wise): NASA/JPL-CalTech/Spitzer

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Presso die vel tempore fasciculum videbis, sicut tunc temporis apparuit.

	Dies/Tempus	Minutio	Dimensiones	Usor	Sententia
recentissima	04:51, 8 Martii 2023		864 × 864 (321 chiliocteti)	Nrco0e	Uploaded a work by X-ray: NASA/CXC/Univ. of West Virginia/H. Blumer; Infrared (Spitzer and Wise): NASA/JPL-CalTech/Spitzer from https://chandra.harvard.edu/photo/2021/j1818/ with UploadWizard

Ad hunc fasciculum nectit:

Quae incepta Vici fasciculo utuntur:

Hic fasciculus alias res continet, saepius a machina originatore additas, et (si fasciculus postea recensus sit) fortasse corrigendas.

Descriptio imaginis	This image contains an exceptional magnetar, a type of neutron star with very powerful magnetic fields. Astronomers have found evidence that this object may be the youngest known magnetar (about 500 years old in Earth's timeframe). It is also the fastest rotating one yet discovered (spinning about 1.4 times per second). This image shows the magnetar in X-rays from Chandra (purple) at the center of the image in combination with Spitzer and WISE infrared data showing the wider field of view. Magnetars form when a massive star runs out of nuclear fuel and its core collapses onto itself.
Auctor	Chandra X-ray Observatory Center
Fons	Chandra X-ray Observatory
Headline	In 2020, astronomers added a new member to an exclusive family of exotic objects with the discovery of a magnetar. New Chandra observations help support the idea that it is also a pulsar.
Credit/Provider	X-ray: NASA/CXC/Univ. of West Virginia/H. Blumer; Infrared (Spitzer and Wise): NASA/JPL-CalTech/Spitzer
Short title	Chandra Studies Extraordinary Magnetar
Usage terms	http://chandra.harvard.edu/photo/image_use.html
Dies et tempus creationis	8 Ianuarii 2021
Orientatio	Normalis
Redactio modi "Exif"	2.31
Spatium colorimetricum	Uncalibrated
Unique ID of original document	1B9BF496E756DA17254E0E2D4D307D74
Date metadata was last modified	07:01, 12 Februarii 2021
Keywords	J1818.0-1607
Contact information	cxcpub@cfa.harvard.edu http://chandra.harvard.edu 60 Garden St. Cambridge, MA, 02138 USA 617.496.7941
IIM version	4