Images | About Gemini | Partners | Jobs | Contact Us |

Main Menu

Public Information & Outreach

Observing With Gemini

Observing Schedules

Gemini Science Archive

Gemini Captures Close Encounter of Jupiter's Red Spots

Print

Thursday, 20 July 2006

Page 1 of 2

Image Release

For release on July 20, 2006

For more information, please contact:

Peter Michaud
Gemini Observatory
Hilo, Hawai'i
(808) 974-2510 (Desk)
(808) 937-0845 (Cell)

Gemini Observatory ALTAIR Adaptive Optics Image

Gemini North adaptive optics image of Jupiter and its two red spots (which apppear white because this is a near-infrared image; in visible light they appear reddish). In this color composite image, white indicates cloud features at relatively high altitudes; blue indicates lower cloud structures; and red represents still deeper cloud features. The two red spots appear more white than red, because their tops hover high above the surrounding clouds. Also prominent is the polar stratospheric haze, which makes Jupiter bright near the pole (unlike the other orange/red features in this image, the polar haze is high in Jupiter's atmosphere). Other tiny white spots are regions of high clouds, like towering thunderheads. In visible light Jupiter looks orangish, but in the near-infrared the blue color is due to strong absorption features. The blue mid-level clouds are also closest to what one would see in a visual light image.

See technical details below for information on processing and techniques used to produce this image.
Full-Resolution TIFF | 2.0mb
Full-Resolution JPEG | 164kb

A high-resolution image released today by the Gemini Observatory shows Jupiter's two giant red spots brushing past one another in the planet's southern hemisphere.

The image was obtained in near-infrared light using adaptive optics which corrects, in real-time, for most of the distortions caused by turbulence in Earth's atmosphere. The result is a view from the ground that rivals images from space.

In the near-infrared, the red spots appear white rather than the reddish hue seen at visible wavelengths.

"It was tricky getting this image," said Gemini astronomer Chad Trujillo who helped lead the effort to capture the event. "Since we used adaptive optics we needed a star-like object nearby to guide on, so we had to find a time when Jupiter's moon Io would appear close enough to Jupiter and the red spots would be optimally placed on Jupiter's disk. Fortunately it all worked out on the evening of July 13th and we were able to capture this relatively rare set of circumstances," said Trujillo.

Both red spots are massive storm systems. The top of the larger one, known for a long time as the Great Red Spot, lies about 8 kilometers (5 miles) above the neighboring cloud tops and is the largest hurricane known in the solar system. The smaller storm (officially called Oval BA, but informally known as Red Spot Junior) is another hurricane-like system. Since it appears nearly as bright as the Great Red Spot in near-infrared images, Red Spot Junior may be at a similar height in the Jovian atmosphere as the Great Red Spot.

Chris Go with Gemini Altair data

Image produced by Chris Go from Gemini adaptive optics data of Jupiter. Listen to the podcast for details on his techniques. This image uses sharpening techniques to enhance details.

Full-Resolution TIFF | 6.0mb
Full-Resolution JPEG | 44kb

Red Spot Junior is roughly half the size of its famous cousin, but its winds blow just as strong. This mighty new storm formed between 1998 and 2000 from the merger of three long-enduring white ovals, each a similar storm system at a smaller scale, which had been observed for at least 60 years. But it was not until February 27th of this year that Philippine amateur astronomer Christopher Go discovered that the color of the newly formed white oval had turned brick red. Astronomers were witnessing the birth of a new red spot.

No one is certain why this white oval turned red. However, University of Hawai'i astronomer Toby Owen supports a hypothesis developed by New Mexico State University astronomer Reta Beebe, who suggests that the merger of the three white ovals led to an intensified storm system. This made it strong enough to dredge up reddish material from deeper in the atmosphere. As this material welled up in the middle of the spot, it is contained (or protected) from escape by the strong circulating currents at the spot's edges. "What's frustrating is that we don't know what this reddish material is," Owen said. "But it appears that the ability to dredge it up depends on the size of these oval storm systems."

Another popular hypothesis contends that the material dredged up from below Jupiter's visible clouds climbs to an altitude where the Sun's ultraviolet light chemically alters it to give it a reddish hue.

Jupiter's Red Spots - A Primer

The Great Red Spot is truly enormous. Its size ranges from about 25,000 to 40,000 kilometers (15,500 to 25,000 miles) in its longest dimension (large enough to contain two to three Earths) and packs wind speeds of 560 kilometers/hour (350 miles/hour). Unlike hurricanes on Earth, which can dissipate over land in a matter of days, Jupiter's Great Red Spot is a product of strong convection currents that violently swirl gases in that region of the planet's atmosphere. It has probably persisted for centuries. First definitely recognized in 1879, the Great Red Spot appears identical to the "Permanent Spot" recorded on Jupiter in 1665 by Jean-Dominique Cassini I (1625-1712) in Italy and may be related to a spot noted by British observer Robert Hooke (1635-1703) in 1664. If so, the Great Red Spot has endured for at least 350 years. Jupiter has no solid surface that would deprive the storm of its condensing "fuel."

The formation of a new red spot on Jupiter, however, may also indicate a climate change on the planet. A recent study by Amy Simon-Miller (NASA-Goddard Space Flight Center) and Imke de Pater and Philip Marcus (University of California, Berkeley) shows that Red Spot Junior is gaining altitude. This indicates a temperature increase in that region. Marcus says that the relatively uniform temperature of Jupiter, where the temperatures at the poles are nearly the same as they are at the equator, is due to the chaotic mixing of heat and airflow from vortices in the planet's atmosphere. But Marcus predicted that the movement of heat from Jupiter's equator to its south pole would nearly shut off at 34˚ southern latitude. This is the same latitude where Red Spot Junior is located. This region may now be acting like a barrier that prevents the mixing of heat and airflow. If it is, Jupiter's equatorial regions will become warmer and its poles will become cooler. Consequently, the planet's average temperature at some latitudes could change by as much as 5.5 degrees Celsius (10 degrees Fahrenheit).

Nothing dramatic is expected to happen as the two storm systems continue their close encounter. The white ovals from which Red Spot Junior is made have passed by the Great Red Spot countless times as the atmospheric current in which they are embedded moves at a different speed from the one at the latitude of the Great Red Spot. Nevertheless, we should keep open the possibility that the Great Red Spot could now, or in the future, push Red Spot Junior into a southern jet stream that is blowing against the storm's counterclockwise rotation. If Red Spot Junior's spin slows, its color may revert back to white, but that remains to be seen. Right now, as the Gemini image shows, Red Spot Junior is demonstrating its staying power.

Each red spot is rotating with Jupiter at slightly different rates and over time, like passing cars on a highway, the two spots change relative positions causing periodic close passages like this. However, this is the first such passage since the new, smaller red spot intensified and turned red. A recent optical image from the Hubble Space Telescope was obtained in April of this year when the two spots were still separated by a considerable distance.

The Gemini image was produced by Travis Rector of the University of Alaska Anchorage, Chad Trujillo of Gemini Observatory and the Gemini ALTAIR adaptive optics team.

Technical Data:

Near-infrared image of Jupiter obtained on the night of July 14, 2006 (UT, July 13 HST) using the Gemini Near-Infrared Imager (NIRI) in conjunction with ALTAIR, the natural/laser guide star adaptive optics system (in natural guide star mode, with field lens) on the Gemini North telescope on Mauna Kea in Hawai'i.

Original data are available for downloading by scientists and amateurs at the Gemini Science Archive

Note: Registered users can obtain data by sorting on UT date (July 14) and Science Program: GN-2006A-DD-2

Field of view: 41 arcseconds

Orientation: north up, east left

Some image contrast enhancement was applied to this image using the "Smart Sharpening Filter" in Adobe Photoshop (registered). See original image here

Filter	Color	FWHM	Exposure Time
Paschen-Beta	Blue	N/A	9 x 0.7 seconds
Methane - Long	Green	N/A	9 x 1.3 seconds
K (2.2 microns)	Red	N/A	9 x 2.0 seconds

Podcasts

Subscribe to our podcast rss feed.

Listen to an interview with amateur astronomer Chris Go and Gemini astronomer Chad Trujillo. AAC Audio File (12:59 | 6.9MB)

How to use Gemini Observatory's podcast with iTunes:

Open iTunes
Select Menu > Advanced > Subscribe to Podcast
Enter the following in the url field: http://www.gemini.edu/services/rss/podcasts.xml

<< Start < Previous 1 2 Next > End >>

Gemini is an international partnership managed by the Association of Universities for Research in Astronomy under a cooperative agreement with the National Science Foundation.

The Gemini Observatory provides the astronomical communities in each partner country with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. in addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the UK Science and Technology Facilities Council (STFC), the Canadian National Research Council (NRC), the Chilean Comisión Nacional de investigación Cientifica y Tecnológica (CONiCYT), the Australian Research Council (ARC), the Secretaria de Ciencia, Tecnología e Innovación productiva (SECYT) and the Brazilian Ministério da Ciência e Tecnologia (MCT). The Observatory is managed by the Association of Universities for Research in Astronomy, inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.

Please read the Gemini image/Video Usage Policy if you wish to use Gemini images and videos.