Friday, 27 November 2020

VOYAGERS TRAVELS

 (6) Voyager 1 has now left our solar system! The news we have been waiting all year to hear has finally been announced, Voyager 1 has entered interstellar space.




Scientists claim Voyager 1 entered interstellar space more than a year ago. Study claims Voyager 1 left the heliosphere around the 25th of August 2012. The reason for the delay in the announcement was because they wanted to be certain, all the data needed to be checked. After careful analysis, scientists are confident that Voyager 1 has left our solar system and is now the first mission to explore interstellar space, the space between our star and the next. Interstellar simply meaning in between stars. 

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Voyager 1 and 2 were built by NASA's Jet Propulsion Laboratory in Pasadena, California, to explore the outer planets of our solar system. Each spacecraft held a self-contained system that carried its own power generation system, propulsion system, communication equipment, and scientific instruments. The primary mission was the exploration of Jupiter and Saturn, including a close look at Saturn's rings and the larger moons of the two planets. Voyager 2 was supposed to act as a backup to Voyager 1. If Voyager 1 failed when taking pictures of Jupiter and Saturn, NASA was prepared to alter Voyager 2's path to follow Voyager 1's trajectory. It would cut off the Uranus and Neptune option, but still, preserve the possibility of some pictures. The mission was intended for five years, but after a succession of fascinating images returned by Voyager, NASA decided to extend the mission. This new mission was to explore the outer planets of our solar system and then eventually to go on and enter interstellar space.

On the 20th of August 1977, Voyager 2 was the first to launch, followed by Voyager 1 sixteen days later. Even though Voyager 2 was launched earlier, Voyager 1 had a faster flight path and arrived at Jupiter four months before its sister craft.

THE GOLDEN RECORD

Onboard Voyager 1 and 2 NASA placed a message, kind of a time capsule, intended to communicate a story of our world to extraterrestrials.

The Voyager message is carried by a phonograph record, a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth. The contents of the record were selected by a committee chaired by Carl Sagan of Cornell University. Dr. Sagan and his associates assembled 115 images and a variety of natural sounds, such as those made by surf, wind, and thunder, birds, whales, and other animals. To this, they added musical selections from different cultures and eras, and spoken greetings from Earth-people in fifty-five languages, and printed messages from President Carter and U.N. Secretary-General Waldheim. Each record is encased in a protective aluminum jacket, together with a cartridge and a needle. Instructions, in symbolic language, explain the origin of the spacecraft and indicate how the record is to be played. The 115 images are encoded in analog form. The remainder of the record is in audio, designed to be played at 16-2/3 revolutions per minute. It contains the spoken greetings, beginning with Akkadian, which was spoken in Sumer about six thousand years ago and ending with Wu, a modern Chinese dialect. Following the section on the sounds of Earth, there is an eclectic 90-minute selection of music, including both Eastern and Western classics and a variety of ethnic music.

Now Voyager has left our solar system, it will be forty thousand years before it makes a close approach to any other planetary system. As Carl Sagan has noted, "The spacecraft will be encountered and the record played only if there are advanced spacefaring civilizations in interstellar space. But the launching of this bottle into the cosmic ocean says something very hopeful about life on this planet."
This picture was taken by Voyager 2 on the 18th of September 1977.  The image of crescent earth was the first of its kind ever taken by a spacecraft. The Earth is many times brighter than the moon so the moon was artificially brightened so that both bodies would show clearly in the prints. At this point, Voyager was 7.25 million miles from Earth. 

5th March 1979 - Voyager 1 makes its closet approach to Jupiter

9th July 1979 - Voyager 2 makes its closet approach to Jupiter

JUPITER

This stunning image of Jupiter captured by Voyager 1 shows its moons, Io on the left, and Europa on the right.




Image taken from Voyager 1

This image captured by Voyager 2 shows Io. 






Image taken from Voyager 2

A closer image was taken showing Jupiter's Great Red Spot. Altogether the Voyagers took over 33,000 pictures of Jupiter and its five major moons.


Jupiter is the fifth planet from the sun and is a gas giant, the biggest planet in our solar system. It is more than twice the size of all the other planets combined, and if it was 80 times more massive, it would have become a star rather than a planet. Jupiter is made up mostly of hydrogen and helium, with small amounts of methane, ammonia, hydrogen deuteride, ethane, water, ammonia ice aerosols, water ice aerosols, and ammonia hydrosulfide aerosols. The most obvious feature of Jupiter is of course its Great Red Spot, a giant hurricane of gases swirling around constantly. At its widest, the Great Red Spot is three times the diameter of the Earth, and its edge spins counterclockwise around its center at a speed of about 225 miles (360 kilometers) per hour. Its magnetic field is nearly 20,000 times stronger than Earth's magnetic field.

Astronomers have been looking at this giant planet for more than 300 years, from the earth, but now we could get up close and personal with the aid of the Voyager spacecrafts. What we now understand about Jupiter is that important physical, geological, and atmospheric processes go on in the planet, its moons, and magnetosphere that were new to scientists.

The biggest surprises came from Jupiter's many moons, one in particular, Io, the discovery of active volcanism on the surface.  It appears that activity on Io affects the entire Jovian system. Io seems to be the primary source of matter that is apparent throughout the Jovian magnetosphere, (the region of space that surrounds the planet). Sulphur, oxygen, and sodium, erupted by Io's volcanoes and spurted off the surface by the impact of high-energy particles, were detected at the outer edge of the magnetosphere. Particles of the same material are also present inside Io's orbit.

For me, the most exciting moon is Europa, instantly recognizable by its cracked surface made of ice. Scientists believe that this moon may hold water underneath its cracked surface, and it is the movement of the water that causes the ice to crack. This might just be the place in our solar system, where life may have taken hold.
 
Europa - One of Jupiter's moons

The colourful image came from Voyager 2 during its close encounter on 9th July 1996. Voyager 2 took many detailed images of Europa. One scientist famously said, "the moon looked as smooth as a billiard ball."

Continuing on their journey, by using the powerful gravity field of Jupiter, both spacecrafts hurled it selves on to Saturn.

12th November 1980 - Voyager 1 flies by Saturn

25th August 1981 - Voyager 2 flies by Saturn

SATURN


Image of Saturn taken by Voyager 1

In this image of Saturn captured by Voyager 1, on the 3rd of November 1980, at a range of just under 8.1 million miles we see Saturn's moons Tethys and Dione.


Image of Saturn taken by Voyager 1 

On leaving Saturn, Voyager 1 managed to snap this famous picture of the dark side of Saturn, unseen from the position of Earth.


Image of Saturn taken by Voyager 2

This true-color image, captured by Voyager 2, on 21st of July 1981, also shows the moons Dione (the small dot at left) and Rhea (lower right) near Saturn.

URANUS

On January 24, 1986, Voyager 2 has the first-ever encounter with Uranus. It came within 81,500 km (50,600 miles) of the planet's cloud tops. 

Voyager 2 radioed thousands of images and huge amounts of scientific data on the planet, its moons, rings, atmosphere, interior, and the magnetic environment surrounding Uranus.


Uranus, 5.7 million miles from Voyager, 17th of January, 1986.


Uranus has 27 known moons, 14 named. Some are half made of ice. 

Information from:-

Voyager 2's images of the five largest moons around Uranus revealed complex surfaces indicative of varying geologic pasts. The cameras also detected 11 previously unseen moons. Several instruments studied the ring system, uncovering the fine detail of the previously known rings and two newly detected rings. Voyager data showed that the planet's rate of rotation is 17 hours, 14 minutes. The spacecraft also found a Uranian magnetic field that is both large and unusual. In addition, the temperature of the equatorial region, which receives less sunlight over a Uranian year, is nevertheless about the same as that at the poles.



Uranus's 5 largest moons Miranda, Ariel, Umbriel, Titania, and Oberon.

The two largest moons are Oberon and Titania. They were first discovered in 1787, by William Herschel and named after Shakespeare's play, A Midsummer Night's Dream. Ariel and Umbriel were the next to be discovered by William Lassell, who had been the first to see a moon orbiting Neptune. They were named after Shakespeare's, The Tempest.

Miranda was discovered in 1948 by Gerard P. Kuiper, at the McDonald Observatory in western Texas. 

In 2014 Noah Hammond, a planetary scientist at Brown University in Rhode Island told Space.com, "Miranda has a really bizarre, deformed surface. It's a really beautiful and exotic moon."



Voyager 2 discovered 10 more moons within a month of arriving at Uranus. 


Voyager 2 image shows Uranus's moon Puck. 

Puck was discovered in December 1985 in images sent back by Voyager 2, during its flyby of Uranus. Puck is named after a mischievous sprite in William Shakespeare's, A Midsummer Night's Dream.

On January the 25th, 1986, Voyager 2 took this farewell shot of the crescent of Uranus, from 600,000 miles away.



Voyager 2 shows the crescent of Uranus

NEPTUNE 


Voyager 2's view of Neptune, 57,000,000 kilometers (35 million miles) away.

On the 25th of August, 1989, Voyager 2 became the first spacecraft to observe Neptune. 

Neptune is a gas giant, along with Jupiter, Saturn, and Uranus. They have no solid surface but possess huge atmospheres. 

Voyager 2 returned the first colour images of Neptune.


Colour image of Neptune, taken by Voyager 2 in 1989

Voyager 2 traveled 12 years at an average velocity of 19 kilometers a second (about 42,000 miles an hour) to reach Neptune, which is 30 times farther from the Sun than Earth is. Voyager observed Neptune almost continuously from June to October 1989.

The average temperature on Neptune is about minus 200 degrees Celsius (minus 392 degrees Fahrenheit). 


Neptune's Rings


The storm system on Neptune rotates counterclockwise.

Neptune has 14 known moons, one being Triton.


Neptune's moon Triton



A parting view of Neptune and moon Triton, taken by Voyager 2

LEAVING OUR SOLAR SYSTEM

Voyager 2 followed a course below the ecliptic plane and headed out of the solar system. NASA renamed the mission, Voyager Interstellar Mission and put Voyager 2's instruments into low power mode to conserve energy.

Voyager 1, on leaving our solar system, turned and took one final image, the famous Pale Blue Dot. The pale, blue dot is Earth.


Voyager 1's Pale Blue Dot


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