Showing posts with label Jovian eclipse. Show all posts
Showing posts with label Jovian eclipse. Show all posts

Wednesday, February 29, 2012

The Rare Triple Eclipse of Jupiter

Written by Matthew Winter 

On March 28, 2004, The Hubble Space Telescope snapped an amazing picture of the transit of two of Jupiter’s confirmed sixty-six moons, and the shadows of three of them, resulting in an image of which shows the spontaneous phenomena capable of this planet’s lunar bodies. At first glances, Jupiter appears to be a brightly colored orb, with hues parallel to a pastel or neon painting, with five different spots placed randomly about its northern hemisphere; its altered coloring was result of being taken by Hubble’s Near Infrared Camera and Multi-Object Spectrometer, instead of photographing in the visible spectrum. The image is comprised of three of these near-infrared photographs, producing the different shades of color visible—yellow indicates high cloud cover, red indicates low, and blue, even lower cloud cover. 


 Although phenomena such as the event captured in the image, finding Jupiter in the night sky is no hard task and can be especially bight when at opposition. But, there are no definite set of celestial coordinates in locating this planet, because of its ever-changing position in the night sky. According to ephemerides however, computers have been able to plot the course of Jupiter on timescales greater than one millennium, so locating and charting the planet’s position will never be tedious work. For the end of February 2012, Jupiter will be visible in the south-southwestern sky just after sunset, at the averaged Right Ascension of 2h 19m and the Declination of + 12° 53’. Again, phenomena seen in the image are rare and do not occur often.

Upon looking at the image, you might inquire of when such an event will occur on Jupiter. Although it might seem very rare that three moons cast their shadow while two transit, rather it is not. This event is called a Jovian Dual-Transit, as it incorporates two different moons, in this case Io and Ganymede, simultaneously transit the surface. But because of the two shadows also cast by these two moons, it is more appropriately named A Jovian Dual-Shadow Transit where two moons transit and cast shadows. The third shadow, consequently given by Callisto, not pictured in the image, makes this event even more complex—and it is quite spectacular that Hubble was in the right place at the right time to photograph such a spectacle. In describing it, however, it is not troublesome to locate the three, distinct shadows of the three moons notwithstanding Io and Ganymede, which seem to be camouflaged in with Jupiter’s pallid colors. Io sits nearly in the center of the image, in white, opposed to its visible color of hazy yellow or golden. Ganymede is to the upper right of Io, and is pale blue; Ganymede is visibly the color of our Moon, a flushed grey.

Whereas a beautiful image of Jupiter with three shadows and two moons cresting its upper hemisphere is rather somber and dreamy, to astronomers, this image allowed them to attempt a new technique of imaging, which succeeded in the end. Attempting to capture images of Jupiter and its moon is rather difficult, especially when completely focused on an object. Because Jupiter moves quickly across Hubble’s telescope view, it was necessary to take a rapid succession of images, before Jupiter moved out of the telescope’s lenses.

Of course, Hubble has the equipment to track an object far away and hold for hours; Jupiter is much closer to earth than distant galaxies, so things tend to move quicker than you would think—and when locked onto it, the sharpness of the image was distorted, creating a blurry picture, not fit to be called a Hubble image. So, astronomers tried, for the purpose of creating a sharper, neater image, to speed up Hubble’s tracking system, resulting in the ‘slower’ movement of Jupiter through the telescope, which in return allowed Hubble to take such a fine image of its moon in such phenomena.

In conclusion, it is important to see that not only did this image of Jupiter’s rare triple ‘eclipse’ phenomena helped astronomers for the better of planetary images (in that, the slowing down of Hubble’s tracking system made clearer photographs of planets from earth), but also to record a rare event for the wonder and mystery of extraplanetary phenomena—other planets do indeed experience eclipses and transits!

With Information from (Accessed February 24 & 27 2012):

Sunday, January 22, 2012

Understanding Jovian Eclipses

[This article concerns Jovian eclipses, not transits. Although a Jovian eclipse can mean the same thing as a transit in this sense, this article talks about the disappearance and reappearance of the Jovian moons, not the transit of Jupiter’s surface.]

Considered the most intriguing and fascinating astronomical phenomena yet, the eclipse is highly acclaimed not just here on earth, but also in the rest of our solar-system. When a celestial body passes into the shadow of another body, preferably larger; or an object casts a shadow upon another, an eclipse is formed. From there, the term ‘eclipse’ can be forwarded into two separate definitions: the solar eclipse, or the lunar eclipse. When the Moon passes in front of the Sun, respectively on the ecliptic, a shadow is cast upon the earth; a solar eclipse is formed. When the Moon passes into either the umbral or penumbral shadow of the earth, again respectively on the ecliptic; a lunar eclipse occurs. Although these definitions discreetly define actions in a terrestrial sense, these same exact phenomena occur on the other seven planets in our vast solar-system, but with another name.

When an object passes into the shadow cone of Jupiter, it disappears from view (note the striped moon to represent being eclipsed instead of being solid colored, not eclipsed)
The Jovian Eclipse is perhaps one of the most unique extraterrestrial happenings, for it involves one of the many Jovian moons, mainly the Galilean moons, Jupiter, and the Sun; rather just the Moon and earth. Because a solar eclipse and a lunar eclipse have terrestrial definitions and terms, therefore, a Jovian Eclipse is defined as “the passing of a Jovian moon into the shadow-cone of Jupiter where it is eclipsed out of sight, until reappearing.” These eclipses can be total, in which the eclipsed moon is eclipsed indefinitely; or partial, where the eclipsed moon is partially eclipsed. But, you must make note that the Galilean moons (the four most famous moons, which we do know to eclipse) have very little orbital inclinations. With Io, having an inclination of 0.050º, Europa with 0.471º, Ganymede with 0.204º, and Callisto with 0.205º, it is doubted that partial eclipses can occur, because each of the moons’ orbits are so perfectly aligned with Jupiter’s equator; therefore, no partial eclipses. Aside from the types of Jovian eclipses that occur, series of eclipses take place, nevertheless imitating ‘Saros’ here on the earth. Because the moons that do eclipse are rather diminutive compared to Jupiter itself, an observer on Jupiter would not notice much, so a Jovian observer would consider a Jovian eclipse as a phenomena of theoretical interest, or something unimportant to note. Nevertheless, the Jovian moons’ ‘Saros’ is pure academic interest as well.

Seeing a Galilean moon eclipse is an enchanting experience you won’t forget. But, certain requirements are needed for you to observe one; it’s hard for Jupiter to produce such key-viewing times, like the one in 1999. “Jupiter and Saturn returned to the sky in autumn of that year; Jupiter was at its best to view in a long time. Jupiter and its moons were easily observed with a small telescope, and two of three phenomena could easily be seen. Transits and occultations were easy to see, but not so much for eclipses. That’s what makes eclipses so amazing,” Matthew Winter writes from Astronomical Events: Eclipses, Transits, Occultations, and Conjunctions. In order for Jupiter to produce a good eclipse viewing season, it first must be at either eastern or western quadrature. Quadrature is simply a fancy term for the time when a planet forms a right triangle with the earth and Sun. Western Quadrature occurs when the planet is towards the west of earth, and Eastern Quadrature is vice versa. Jupiter forms a twelve degree angle on its end, while the ninety degree angle is on earth’s end. Then, we are able to see the moons eclipse in and out of Jupiter’s shadow cone, rather than at opposition. At opposition, when the earth, Sun, and the planet of note (Jupiter) are all aligned in a straight line, Jupiter’s shadow cone is behind the planet, making eclipses invisible from earth. Precise timings are location is everything in viewing a Jovian eclipse. “Because its shadow cast is very magnificent, when a Galilean moon passes behind it, it disappears completely from view, but has not been occulted. As well as that, because the shadow cast is so steep, the Galilean moons may be viewed entering and exiting the shadow on the same side of the planet!,” from Astronomical Events: Eclipses, Transits, Occultations, and Conjunctions.

Jupiter’s shadow cone is brought into our view at quadrature, it’s not at opposition, which is when Jupiter would make the earth, Sun, and Jupiter in a straight line.
August 1, 2011 brings us to Jupiter’s Western Qudarature, which is a key time to view these events. Around west quadrature, Jupiter rises beautifully in the east around midnight and shines high up at dawn. But mind you, Jupiter takes over eight years to orbit, so returning to Eastern Quadrature will take a few years, so patience is a good aspect in waiting for the return of the Jovian eclipses.  Returning to 1999, Capitol Skies (the newsletter of the Madison Astronomical Society) tells us this about the Jovian eclipses during that epic season. “Jupiter provides a virtual smorgasbord of events to watch. Of the three events, eclipses are by far the most scientifically interesting, because the timing of the precise disappearances and reappearances of the moons can be used to calculate orbital elements of the moons. For this reason, precise timings of the Galilean moon eclipses are sought by the Association of Lunar and Planetary Observers (ALPO).” You can visit a myriad of online resources to locate the times of Jovian eclipses, for what more is there to miss? A moon may be eclipsing now!

Here is a basic explanatory site of Jupiter’s phenomena:

Galilean moons simulator from the Transits Page (click ‘now’ for most current events):

[To download the Word Document of this story, come to this page where it can be downloaded.] 
 
http://astronomicaleventscalendar.blogspot.com/2011/08/understanding-jovian-eclipses.html 

Tuesday, October 25, 2011

Results of the October 24, 2011 Jovian Dual Transit

The dual-shadow transit on October 24, this past Monday was a true spectacle! Although we here in America could not view such a wonderful event, I have been able to find a few pictures scattered across the internet of this spectacular event. About the transits: "After having such a prolific season of simultaneous Jovian dual-transits last May-June, it will be hard to accept the fact that we have only two more this 2011 season: October 24, 2011 and October 31, 2011. Each transits are an exact week apart (although times differ) and both are dual-shadow transits. Io and Ganymede both partake in each event, as their orbits must be aligned perfectly just for this week." Read more at the link above.

This picture was taken from 'Cloudy Night Telescope Reviews' under username 'claytonbigwood'

Below is a picture computed (simulated) by Celestia software. You can see Ganymede and Io as the light blobs, and their shadows cast on the planet. If you would to see the picture clearer, you may click on it for higher resolution.


Although these are not the most high quality images available, they do beautifully illustrate the beauty of this transit. Remember that October 31 brings us another galactic delicacy! Another dual-shadow transit awaits us...

Saturday, October 22, 2011

December 27, 2011 Dual-Shadow Transit

According to the "Robert Ferguson Observatory," they state in their 2011 Observing highlights, that there will be a dual-shadow transit of Europa and Ganymede on December 27, 2011. Although I do recommend their observing highlights to those who would like to know, their event is incorrect. They have:

  • Tuesday, 12/27/2011 - Dbl Sh Tr Jup - Time: 18:00
    • Double shadow transit of Jupiter:
      Transit of Europa is already in progress at sunset.
      06:00p Nautical twilight ends
      06:05p Ganymede's shadow begins transit
      06:32p Astro twilight ends
      07:44p Io is occulted by Jupiter
      07:51p Europa's shadow begins transit
      07:52p Europa transit ends
      07:55p Ganymede's shadow transit ends
      10:15p Europa's shadow transit ends
      11:07p Io reappears from eclipse

Although I do not wish to refute this prediction, after checking the Galilean moons simulator, they're prediction is wrong. Ganymede does transit and Io does eclipse, but Europa is just too far away from Ganymede for dual-shadow transit. Without making any advanced Judgments, this may occur, but maybe if viewed from a different angle on the earth.

Computer Simulation of Galilean moons provided by the Galilean Moons Simulator, Text Inserted by AstronomicalEventsCalendar


Credit: NASA