Images from the Hubble Space Telescope's Faint Object Camera from 1991, 1992, and 1993 demonstrate motion in the R Aquarii emission jet. Since images from this period were still affected by the primary mirror flaw, the images were restored to the original design resolution using the maximum entropy method.
Please give credit for this item to: NASA/Goddard Space Flight Center
Scientific Visualization Studio
Science Paper: J. M. Hollis, R. G. Lyon, J. E. Dorband, W. A. Feibelman, Motion of the Ultraviolet R Aquarii Jet, ApJ, 475, 231-236.
Short URL to share this page: http://svs.gsfc.nasa.gov/1389
Data Used: HST/FOC
1991/10/21, 1992/12/01, 1993/10/17
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.