File:Millisecond pulsar and accretion disk - NASA animation (hi-res).ogv
Millisecond_pulsar_and_accretion_disk_-_NASA_animation_(hi-res).ogv (Ogg Theora video file, length 47 s, 640 × 480 pixels, 3.09 Mbps, file size: 17.4 MB)
Captions
Captions
Summary
editDescriptionMillisecond pulsar and accretion disk - NASA animation (hi-res).ogv |
English: Animation showing neutron star and accretion disk evolving into a millisecond pulsar, with magnetic fields.
The formation of a pulsar: A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. Deutsch: Animation: Die Entstehung eines Pulsars:
Ein Stern in einem Doppelsternsystem kollabiert zu einem Neutronenstern. Es beginnt Material von seinem Begleiter zu ihm zu strömen (Akkretion). Die einfallende Materie verursacht eine Beschleunigung und das Aussenden hoch-energetischer Strahlung. Schließlich ist ein Pulsar entstanden, der sich bis zu 1000 mal pro Sekunde dreht. Čeština: Animace vzniku pulsarů
|
Date | |
Source |
Millisecond pulsar and accretion disk - NASA animation (hi-res).ogv http://svs.gsfc.nasa.gov/vis/a010000/a010100/a010144/index.html |
Author | NASA (animator: Dana Berry) |
Other versions |
File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv See also other versions on NASA pages |
File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv
File:Millisec xray pulsar H.jpg (still frame)
See also other versions on NASA pages
![]() |
This file was selected as the media of the day for 13 May 2011. It was captioned as follows:
English: Animation: the formation of a pulsar
A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. Other languages
Čeština: Animace vzniku pulsarů Deutsch: Animation: Die Entstehung eines Pulsars Ein Stern in einem Doppelsternsystem kollabiert zu einem Neutronenstern. Es beginnt Material von seinem Begleiter zu ihm zu strömen (Akkretion). Die einfallende Materie verursacht eine Beschleunigung und das Aussenden hoch-energetischer Strahlung. Schließlich ist ein Pulsar entstanden, der sich bis zu 1000 mal pro Sekunde dreht. English: Animation: the formation of a pulsar
A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. |
Licensing
editPublic domainPublic domainfalsefalse |
![]() |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ![]() |
![]() |
Warnings:
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 15:14, 8 May 2011 | 47 s, 640 × 480 (17.4 MB) | FT2 (talk | contribs) | == {{int:filedesc}} == {{Information |Description ={{en|1=Animation showing neutron star and accretion disk evolving into a millisecond pulsar, with magnetic fields.}} |Source =Millisecond pulsar and accretion disk - NASA animation (hi-res). |
You cannot overwrite this file.
File usage on Commons
The following 9 pages use this file:
- File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv (file redirect)
- Template:Motd/2011-05
- Template:Motd/2011-05-13
- Template:Motd/2011-05-13 (cs)
- Template:Motd/2011-05-13 (de)
- Template:Motd/2011-05-13 (en)
- Template:Motd/2011-05-13 (zh-hans)
- Template:Potd/2011-05 (zh-hans)
- Category:Millisecond pulsars
Transcode status
Update transcode statusFile usage on other wikis
The following other wikis use this file:
- Usage on ar.wikipedia.org
- Usage on az.wikipedia.org
- Usage on bn.wikipedia.org
- Usage on ca.wikipedia.org
- Usage on de.wikipedia.org
- Usage on en.wikipedia.org
- Usage on fa.wikipedia.org
- Usage on fr.wikipedia.org
- Usage on it.wikipedia.org
- Usage on ka.wikipedia.org
- Usage on kk.wikipedia.org
- Usage on lb.wikipedia.org
- Usage on ml.wikipedia.org
- Usage on mn.wiktionary.org
- Usage on mr.wikipedia.org
- Usage on my.wikipedia.org
- Usage on oc.wikipedia.org
- Usage on ru.wikipedia.org
- Usage on sv.wikipedia.org
- Usage on ta.wikipedia.org
- Usage on tt.wikipedia.org
- Usage on www.wikidata.org
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.
Software used |
---|