SCIENTIST FOR A DAY 2013 CONTEST ESSAY
DEDICATED TO: The magnificent team of Tv actors(tresses) of the Warner tv program of the same name).
TEAM MEMBERS:                                             SCHOOL:
Luis Manuel Garcia Teran                                    Liceo Los Robles 
Maria Jose Garcia Teran                                       Altamira
Gabriel Moreno                                                     Apamates
Nay Valbuena   (Team Leader)                             Merici
Armando Gutierrez                                                Los Robles
Nestor Bohorquez  (Team Leader)                        Los Robles
Ernesto Gomez    (Team Leader)                           Los Robles
Emanuel Caridad                                                    Urbe San Onofre
Jose Vallejo                                                             Luz
Lermith Biarreta                                                     Los Robles
Maria Frnda Biarreta                                              Altamira
Arturo Negrette   (Team Leader)                            Los Robles
Josue Castro                                                            Feliciano Palacios
Yirrel Castro                                                           Feliciano Palacios Luz
Jonar Cubillan   (Team Leader)                                                      Luz
Jesus Perozo (Team Leader)                                   Los Robles
Manuel Villalobos                                                   Los Robles
Sath Peraza                                                               Los Robles
Barath Peraza                                                           Los Robles
Aria Matos                                                               Altamira
Miguel Bohorquez                                                   Los Robles URU
Andrea Fajardo  (Team Leader)                               Unefa
Estefany Angulo                                                       Unefa
Christian Barrera  (Team Leader)                             Los Robles
Ines Monteverde   (Team Leader)                             Altamira
Diego Nava                                                                Sta Mariana de Jesus 
“ We as a group thought that Iapetus is the best target for photographic investigations assisted by Cassinis  instruments based in a few curious aspects that called our attention because its own particular characteristics, such the moon’s form, location, aspect and  geological history wich indicate there might be amazing forces in action. 
The origin of Iapetus’s dark zone (Cassini Regio) and its ecuador (toledo Montes)* according to the apparent exogen origin of the dark dust Iapetus in its past* attracts our attention because we read*it could be due to this moons orbit close to saturn wich provides it with posible  thermonuclear activity* plus the fact that its inclination was alredy present. This thermonuclear activity posibly made possible that its surface was more exposed to the gravitational activity of its own speed rotation faster compared to the actual speed rotation* posses so in theory*also  its approximation to the rings and the gravitational attraccion that these could cause to the surface might explain the formation of the Himalaya* on its own curious ecuatorial location. We read a theory* that in a distant past the closeness of iapetus to saturn and its outer ring caused its surface  plus the possible its own gravitational activity that could cause it* thanks to its posible active core*wich allows to add particules from saturn’s rings*. About the dark dust, we read  that Iapetus’s  past closer orbit to saturn could made possible a collition with any other defunct moons as well to other any other kind of celestial body, this impact might have  caused the estrangement of its orbit; we read* that in its possible original orbit the moon lost its atmosphere activity allowing the settlement of  particles from a possible past  impact* in one specific region, giving way to the known dark zone. the descent of the surface’s temperature gave way to the solidification of Toledo Montes*. It is possible  the dark dust was in the moon previous to the shining regions suggesting that the last, is a criogenisation process in the dust* not been completely covered maybe for the termic segregation phenomenon present in the dark dust, giving way to the “black spots” in the bright region*.
To analyze the “black spots” we suggest using photography combined with  (CIRS) to know the temperature and composition, proving the thermic segregation process in the bright region*, allowing to recreate  3D map of Iapetus to study the  structure of Toledo Montes.
Combinig photography with (VIMS) we could  study and analyze the nature of the particules that form the Toledo Montes.
And combining with (RADAR) we could create better detailed  maps of Iapetus’s surface. 
We really like it for both reasons: its craters and its  quality of black and white colors that make it look like the Death Star from StarWars.
In the seventeenth century, Giovanni Cassini observed that Iapetus could be seen when it was on one side of Saturn but not the other. He concluded that one of its hemispheres was darker than the other, which was then confirmed through images thanks to Voyager 1 (1981), and Cassini / Huygens closest approach on September 10, 2007.*
Combining photography with Imaging Science Subsystem (ISS) to observe the differentiation of the hemispheres, the Ultraviolet Imaging Spectrograph (UVIS) for spectrographic and scanning profile of the composition of the surface* and have unprecedented coverage that would allow dark material thickness and composition studies.
The dark region is called Cassini Regio and the clear region Roncevaux Terra.
We read 2 theories:*. External origin: suggests that the dark material is not Iapetus origin and that it comes from another moon of Saturn that received a strong impact of a huge meteorite and this material was expelled to Iapetus.
2. Internal origin:* proposes that the dark material comes from within and surfaced through a combination of meteoric impact and cryo-volcanism. It has also been suggested* that the dark regions may  be areas without water.
The equatorial ridge of Iapetus is another photographic aspect; discovered by Cassini/Huygens. Its range is 20 kilometers wide and 13 high, and stretches  1300 kilometers from the dark side. The reason behind this formation  would be another photographic target. We read  several theories.*
• It could be  remnant of  spheroid shape Iapetus in the beginning, when it rotated faster.
• It is composed of a liquid that emanated from sources below the surface and then solidified.
• Might have had its origin in the distant past, when Iapetus would have touched the outermost portion of the rings of Saturn and consumed part of its materials.
• It could be the result of the impact of an Iapetus debris ring created from a sub – satellite rupture that orbited this moon*.
1) Space at the service eof our environment,ESAmFlorence,Italy,14 March 1997
2) Astronomy, by Paul Muller, Paris Observatory
3) JPL website
4) Mysteries of Mind,Space & Time, Websters Home Library
5) Encyclopedia of the Solar System, by, Academic Press
6) The explosion of Science, by Meredith Press
7) Craters ! by Natl Science Teachers association
8) Visions, by Dr Michio Kaku
9) ESA bulletin num 98, june 1999


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    Hello,my name is Patrick Morton, 63 years old,Petroleum Engineer, amateur astronomer,volunteer coordinator for The Planetary Society,JPL Scientist for a day Intl edition contest, volunteer member at Saturn Observation Campaign, volunteer instructor in Venezuela for Project Astro, ASP, actually working as natural sciences and amateur astronomy teacher at Liceo los Robles Elementary and High School, my father was a WW2 pilot officer in the RAF, my mother worked for Shell Oil co,and my brother is an electromnics engineer, my wifes name is Itala, and my daughters name is Daniela, my dogs name is Grecia,I also have 9 cats and i have...


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