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Piú viste - The Universe Inside
Petals.jpg
Petals.jpgPetals on Mars (by Bruce Moyant)90 visitenessun commentoMareKromium
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Metis_and_Jupiter.jpgMetis and Jupiter90 visitenessun commentoMareKromium
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ShatterDay.jpgShatterday (by Roberto Tremolada)90 visitenessun commento1 commentiMareKromium
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Aurora_Borealis-Coronal_Aurora-1.jpg"Auroral Corona" from l'Observatoire de la Dcouverte in Val Belair near Quebec - Canada89 visiteDa "NASA - Picture of the Day" del 9 Novembre 2004: "...This fisheye picture captures a particularly active and colorful 'Auroral Corona' that occurred on November 7, 2004 (...) The above aurora has an unusually high degree of detail, range of colors and breadth across the sky. The vivid green, red, and blue auroral colors are likely caused by high atmospheric oxygen and hydrogen reacting to incoming electrons. The trigger events were magnetically induced explosions on the Sun from sunspot region 696 over the past few days. Continued activity from this active solar region could mean more auroras visible to northern observers over the next few days. Early in the morning but far in the background, planets, stars and the Moon will be simultaneously putting on their own show".
Una piccola (nostra) nota di commento: dietro la vivace bellezza dell'immagine ed i "romantici" commenti, c' un nuovo incremento dell'attivit solare in un periodo in cui, invece, il nostro Sole usualmente calmo.
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ALANBEAN-LUNARROVER.jpgLunar "Grand Prix"89 visiteApollo 16 Commander John Young is putting the Lunar Rover through a full test. This was the second mission with the Rover onboard and this Lunar Grand Prix would allow John to evaluate the performance of the Rover in the light gravity and the dusty, cratered, and rocky surface of the Moon.
His companion, Charlie Duke, is photographing it all with the 16-mm Data Acquisition Camera normally mounted on the Rover, but hand-held temporarily to document the Rover motion.

John later said:"The tendency was to drive wide open or very close to that and take what you got. The best reference to speed control was the speedometer, as I really didn't have a feel for the difference between 7 and 10 Km per hour."
Later, he demonstrated a sharp turn at ax speed, about 10 Km per hour. I made the Rover end break out to show the engineers how it looked.
It is no problem as all I had to do was cut back like I do when driving in snow...I didn't get up to any great speed, maybe 10 clicks at the most, but the terrain around there was too rough and rocky for that kind of foolishness..."

Charlie, who was filming it all, told Houston, "...man, Indy has never seen a driver like this."
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Perseid-1.jpgShooting Star (1)89 visiteL'immagine sicuramente bella, ma quello che vorremmo farVi notare la tessitura della striscia lasciata dalla "stella cadente" la quale, come ben si vede (anche senza operare ingrandimenti), contiene "nodi" (modesti rigonfiamenti dovuti, probabilmente, a perdita/consunzione di materiale a seguito dell'attrito durante la caduta del frammento di Corpo Celeste attraverso l'atmosfera) e "brillamenti" (delle vere e proprie "fiammate" che si avviano, di regola, in corrispondenza dei "nodi" e che indicano cambi di temperatura - ergo di luminosit - del Corpo in questione).
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Aurora_Borealis_-_02.jpgPeaceful Morning Sky89 visitenessun commentoMareKromium
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Voyagers-00.gifTowards the "Terra Incognita" (1)89 visiteInterstellar Mission - Mission Objective

The mission objective of the Voyager Interstellar Mission (VIM) is to extend the NASA exploration of the Solar System beyond the neighborhood of the outer planets to the outer limits of the Sun's sphere of influence, and possibly beyond. This extended mission is continuing to characterize the outer Solar System environment and search for the heliopause boundary, the outer limits of the Sun's magnetic field and outward flow of the solar wind. Penetration of the heliopause boundary between the solar wind and the interstellar medium will allow measurements to be made of the interstellar fields, particles and waves unaffected by the solar wind.
The VIM is an extension of the Voyager primary mission that was completed in 1989 with the close flyby of Neptune by the Voyager 2 spacecraft. Neptune was the final outer planet visited by a Voyager spacecraft. Voyager 1 completed its planned close flybys of the Jupiter and Saturn planetary systems while Voyager 2, in addition to its own close flybys of Jupiter and Saturn, completed close flybys of the remaining two gas giants, Uranus and Neptune.

At the start of the VIM, the two Voyager spacecraft had been in flight for over 12 years having been launched in August (Voyager 2) and September (Voyager 1), 1977. Voyager 1 was at a distance of approximately 40 AU (Astronomical Unit - mean distance of Earth from the Sun, 150 million kilometers) from the Sun, and Voyager 2 was at a distance of approximately 31 AU.

As of July 2007, Voyager 1 was at a distance of 15.4 Billion Kilometers (103 AU) from the sun and Voyager 2 at a distance of 12.4 Billion kilometers (83 AU).

Voyager 1 is escaping the solar system at a speed of about 3.6 AU per year, 35 degrees out of the ecliptic plane to the north, in the general direction of the Solar Apex (the direction of the Sun's motion relative to nearby stars). Voyager 2 is also escaping the solar system at a speed of about 3.3 AU per year, 48 degrees out of the ecliptic plane to the south.


Both Voyagers are headed towards the outer boundary of the solar system in search of the heliopause, the region where the Sun's influence wanes and the beginning of interstellar space can be sensed. The heliopause has never been reached by any spacecraft; the Voyagers may be the first to pass through this region, which is thought to exist somewhere from 8 to 14 billion miles from the Sun. In December 2004 Voyager 1 crossed an area known as the termination shock. This is where the million-mile-per-hour solar winds slows to about 250,000 miles per hourthe first indication that the wind is nearing the heliopause. Voyager 2 is currently observing preshock phenomena, indicating that it is close to the termination shock. The Voyagers should cross the heliopause 10 to 20 years after reaching the termination shock. The Voyagers have enough electrical power and thruster fuel to operate at least until 2020. By that time, Voyager 1 will be 12.4 billion miles (19.9 billion KM) from the Sun and Voyager 2 will be 10.5 billion miles (16.9 billion KM) away. Eventually, the Voyagers will pass other stars. In about 40,000 years, Voyager 1 will drift within 1.6 light years (9.3 trillion miles) of AC+79 3888, a star in the constellation of Ophiucius. In some 296,000 years, Voyager 2 will pass 4.3 light years (25 trillion miles) from Sirius, the brightest star in the sky . The Voyagers are destinedperhaps eternallyto wander the Milky Way. For current distances, check: Mission Weekly Reports

MareKromium
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Venus_and_the_Moon.jpgNight Lovers'...89 visitenessun commentoMareKromium
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Beyond.jpgBeyond... (by Roberto Tremolada)89 visitenessun commento4 commentiMareKromium
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Jupiter_and_Europa.jpgFather and Son (by Roberto Tremolada)89 visitenessun commentoMareKromium
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SettingSun.jpgA Day of the Sun88 visite"...Peace I leave with you; my Peace I give to you..."

- John 14:27

nota: "A Day of the Sun" anche il titolo di una serie di opere dedicate al Sole, realizzate dal Pittore Tetsuro Sawada.
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