Jump to content

Faịlụ:Interferometric astrometry.jpg

Page contents not supported in other languages.
Shí Wikipedia, njikotá édémédé nke onyobulạ

Interferometric_astrometry.jpg (450 × 160 pixel, ívù akwukwo orunótu: 32 KB, MIME nke: image/jpeg)

Failụ a si na Wikimedia Commons,enwekwara ike iji ya eme ihe na arụmarụ ọzọ. Nkọwa na ihuakwukwọ nkọwa failụ eziri na okpuru.

Mmẹkụwátá

Moved This file was moved to Wikimedia Commons from en.wikipedia using a bot script. All source information is still present. It requires review. Additionally, there may be errors in any or all of the information fields; information on this file should not be considered reliable and the file should not be used until it has been reviewed and any needed corrections have been made. Once the review has been completed, this template should be removed. For details about this file, see below. Check now!
Nkówá
English: Retrieved from [1] - JustinWick 21:31, 11 December 2005 (UTC) Illustrates the use of optical wavelength interferometry to determine precise positions of stars.
Ǹgụ́ụ̀bọ̀chị̀ 11 Disemba 2005 (original upload date)
Mkpọlọ́gwụ̀ Transferred from en.wikipedia to Commons by FSII using CommonsHelper.
Odé ákwụ́kwọ́ The original uploader was JustinWick at Bekee Wikipedia.
Nke ya ozor
This diagram image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with {{vector version available|new image name}}.


It is recommended to name the SVG file “Interferometric astrometry.svg”—then the template Vector version available (or Vva) does not need the new image name parameter.
This diagram image was uploaded in the JPEG format even though it consists of non-photographic data. This information could be stored more efficiently or accurately in the PNG or SVG format. If possible, please upload a PNG or SVG version of this image without compression artifacts, derived from a non-JPEG source (or with existing artifacts removed). After doing so, please tag the JPEG version with {{Superseded|NewImage.ext}} and remove this tag. This tag should not be applied to photographs or scans. If this image is a diagram or other image suitable for vectorisation, please tag this image with {{Convert to SVG}} instead of {{BadJPEG}}. If not suitable for vectorisation, use {{Convert to PNG}}. For more information, see {{BadJPEG}}.

Nkwényé

Courtesy NASA/JPL-Caltech

© The copyright holder of this file, NASA/JPL-Caltech, allows anyone to use it for any purpose, provided that the copyright holder is properly attributed. Redistribution, derivative work, commercial use, and all other use is permitted.
Í-kpó-áhà:
Courtesy NASA/JPL-Caltech

Copyright Copyright According to JPL's image use policy additional restriction is that no endorsement of any product or service by Caltech, JPL or NASA is claimed or implied.

Caltech's disclaimer: Caltech makes no representations or warranties with respect to ownership of copyrights in the images, and does not represent others who may claim to be authors or owners of copyright of any of the images, and makes no warranties as to the quality of the images. Caltech shall not be responsible for any loss or expenses resulting from the use of the images, and you release and hold Caltech harmless from all liability arising from such use.

Usage on the English Wikipedia: On the English Wikipedia you can use the {{JPL Image}} template to display the copyright notice. (See w:Wikipedia:Using JPL images for details)

Original upload log

The original description page was here. All following user names refer to en.wikipedia.
  • 2005-12-11 21:31 JustinWick 450×160× (33103 bytes) Retrieved from [http://origins.jpl.nasa.gov/library/ipff/ipff06.html] - ~~~~ Illustrates the use of optical wavelength interferometry to determine precise positions of stars. {{JPL Image Copyright}}

Nkowapụta

Tinye nkọwa otu ahịrị ihe faịlụ a na-anochi anya ya.
Illustration of the use of optical wavelength interferometry to determine precise positions of stars.

Ihe ndị egosiri na faịlụ a

depicts Bekee

Optical Interferometry Bekee

Oge/afọ mmalite

11 Disemba 2005

Ịta nke usòrò

Bìri èhì/ogè k'ị hụ òtù ụ̀fa dị̀ m̀gbè ahụ̀.

Èhì/OgèMbọ-akaÓgólógó na asaáÒjìèmeNkwute
dị ùgbu â03:13, 26 Novemba 2011NvóÁká màkà otù ȯ dị nà 03:13, 26 Novemba 2011450 × 160 (32 KB)File Upload Bot (Magnus Manske) {{BotMoveToCommons|en.wikipedia|year={{subst:CURRENTYEAR}}|month={{subst:CURRENTMONTHNAME}}|day={{subst:CURRENTDAY}}}} {{Information |Description={{en|Retrieved from [http://origins.jpl.nasa.gov/library/ipff/ipff06.html] - [[:en:User:JustinWick|JustinWic

Ihe ndị na-eso ihe eji Ihu akwụkwọ eme na faịlụ a:

Ejiji failụ zụrụ ọha

Wikis ndi a edeputara na eji kwa failụ a:

Ewepụtara na https://ig.wikipedia.org/wiki/Faịlụ:Interferometric_astrometry.jpg