- Captain's Logs
- Feb 23, '22
- Sep 15, '17
- Sep 15, '15
- Jan 14, '15
- Dec 24, '14
- Jul 28, '14
- Jun 30, '14
- Nov 12, '13
- Jun 18, '13
- Dec 18, '12
- Jul 12, '12
- Apr 23, '12
- Nov 17, '11
- Jul 6, '11
- Nov 1, '10
- Sep 21, '09
- May 7, '09
- Apr 2, '09
- Mar 23, '09
- Dec 31, '08
- Nov 1, '08
- Jun 30, '08
- Mar 26, '08
- Dec 24, '07
- Oct 15, '07
- Mar 15, '07
- Dec 29, '06
- Sep 19, '06
- Jun 18, '06
- Mar 9, '06
- Dec 22, '05
- Jun 28, '05
- Jan 11, '05
- Dec 30, '04
- Nov 29, '04
- Oct 26, '04
- Sep 9, '04
- May 6, '04
- Feb 27, '04
- Dec 5, '03
- Nov 13, '03
- Nov 1, '02
- Mar 13, '02
- May 31, '01
- Oct 9, '00
- Feb 11, '00
- Sep 1, '99

|
 |
Tvashtar Composite
 PIA 09359
Image 399 x 852:
JPEG 23 KB
PNG 179 KB
|
|
Variations in the appearance of the giant plume from the Tvashtar volcano on Jupiter's moon Io are seen in this composite of the best photos taken by the New Horizons Long Range Reconnaissance Imager (LORRI) during its Jupiter flyby in late February-early March 2007.
New Horizons was fortunate to witness this unusually large plume during its brief Jupiter flyby; the Galileo Jupiter orbiter spent more than five years imaging the volcanic moon (between 1996 and 2001) without ever capturing such detailed pictures of a large Io plume. The plume is roughly 330 kilometers (200 miles) high. The cause of the fine wispy structure in the plume, which varies strikingly from image to image, is unknown, but these pictures may help scientists to understand the phenomenon.
The pictures were taken at distances ranging from 3.1 to 2.3 million kilometers (1.9 to 1.4 million miles), but they have been scaled to show the plume at the same relative size in every frame. Illumination conditions also vary: in the final image, Io's shadow cuts across the plume and hides all but its topmost regions, and the glow of hot lava can be seen on the nightside at the source of the plume. The times of the images, from top to bottom, are: February 26, 18:38 (Universal Time); February 26, 21:01; February 28, 03:50; February 28, 04:40; February 28, 11:04; and March 1, 00:35.
Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute |
|