In Space News 2017-06-13T21:44:41+00:00
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Rosetta - On September 30, 2016, the Rosetta Spacecraft joined the Philae lander on the surface of Comet 67P. Scientists found evidence of organic compounds on the comet that could explain how life on earth began

Extremes on Planet Earth

June 13, 2017

Hottest and Coldest: In 1922, a weather station in El Azizia, Libya recorded the temperature on September 13, 1922 to be 136 F (57 C), while the coldest place on earth was -128 C (90 C) logged by Russian scientists at a research lab in Antarctica on July 20, 1983

Highest and Lowest: Mt. Everest is known as the tallest mountain above sea level. It’s 29,029 ft (8,848 m) summit is rising approximately 2 inches per year. The deepest point below sea level is 39,070 ft (10,994 m) within the Mariana trench

Largest earthquake in the U.S:  On March 28, 1964, a magnitude 9.2 jolted Prince William Sound, Alaska. …in the world:  A 9.5 quake shook Chile on May 22, 1960 followed by powerful tsunamis that killed thousands

Deadliest hurricane in the U.S:  Though we might guess Katrina in 2005, that was a category 3 storm compared to a category 4, the Great Galveston Hurricane, which struck Texas in September of 1900. …in the world:  In November 1970, a category 3 typhoon leveled the western coast of both India and Pakistan, killing 300-500,000


Read Instride: The Earth


Deep Space Network

June 18, 2017

The Jet Propulsion Laboratory in California is NASA’s home base for unmanned space travel. Scientists of the JPL oversee missions such as the Opportunity and Curiosity rovers on Mars, the Juno spacecraft orbiting Jupiter, and the Cassini mission exploring Saturn. 

The Jet Propulsion Labs are also where NASA’s Deep Space Network is managed. The “network” is a series of dish-shaped antennas at three strategic locations around the globe; California, Madrid, and Australia. The stations are spaced approximately 120 degrees longitude apart from each other, ensuring that as the earth rotates there is a continual connection with NASA spacecraft wherever they are in the solar system.

Using the Deep Space Network, a spacecraft orbiting millions of kilometers away can be repositioned as NASA scientists send commands to change its speed and trajectory. When a spacecraft finishes the research it was tasked for, missions are often extended. Software upgrades can be transmitted to the spacecraft, sending it off in another direction within the solar system.

Spacecraft in turn “communicate” with NASA about the complex systems that keep them in flight, while transmitting detailed images from other worlds … the planets, moons, and asteroids that might otherwise never be seen from Earth.

Read Instride: The Solar System

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Mars Rocks!

May 9, 2017

When meteorites from space are found on earth, scientists can usually determine where they came from based on information about the atmosphere and geology of the other terrestrial planets. 

An example in recent years is the meteorite NWA7034, found in the Sahara Desert in 2011. Scientists not only classified it as having originated on Mars, they theorize it is more than two billion years old and contains more water than other “younger” meteorites known to have come from the red planet. 

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Read Instride: Mars


Mercury's Elliptical Orbit

April 14, 2017

About four and a half billion years ago, the gravitational pull of the newly formed sun influenced the location of the planets within the solar system. Each one eventually settled into a stable orbit, traveling on paths that range from near circular to oval. 

A circular pathway through the solar system, such as the one Venus travels on, means that a planet is orbiting the sun at a constant distance and speed. Planets with an elliptical orbit, like that of Mercury, were formed with a speed and trajectory that is continually changing.

At perihelion (nearest the sun) Mercury speeds up and then “sling shots” away, slowing down at aphelion (farthest from the sun) before being pulled in again by gravity.


Read Instride: Mercury


Lava Plains on Venus

February 20, 2017

Venus and the Earth are similar in that they both have a molten core that erupts at the planet’s surface.

On Earth, the most familiar type of volcanoes are the composite type, the cone-shaped structures that explosively spew lava, ash, and hot gases from a chamber of molten rock beneath the surface. They’re usually located along fractures in the earth’s crust where tectonic plates are clashing, such as the ring of fire that includes Mt. St. Helens in the northwestern US.

Shield volcanoes, in contrast, are like the ones found in the Hawaiian Islands, characterized by a continuous and steady flow of lava that cools to reshape the landscape.

Because of Venus’ heavy atmosphere and lack of tectonic plates, its volcanoes are the shield type from which molten rock slowly and uneventfully flows to create the lava plains and “pancake” domes that cover the planet.

Read Instride: Venus


Earth's Moon

February 11, 2017

In recent years, China, Japan, India, the ESA, and NASA have all been exploring the moon. They’ve conducted flybys, placed spacecraft in orbit, and the Chang’e 3 was the first lander on the moon since 1976.

The Lunar Reconnaissance Orbiter is a NASA mission launched in June 2009. The LRO arrived at the moon after a four day journey and was placed in orbit approximately 30 miles (50 km) above the surface. With specialized equipment, NASA has been creating a 3D map of the landscape while collecting data about the effects of the sun’s radiation in space and searching for water ice at the north and south

Using images from the LRO, NASA has created a tour of the moon with an overview of its largest impact craters and evidence that volcanos erupted at the surface of the moon billions of years ago.

Read Instride: Earth's Moon


Exploring Titan

February 7, 2017

The Huygens lander, part of NASA’s Cassini mission, bounced and tumbled on the surface of Titan in January 2005 and then transmitted data through the Cassini orbiter and back to earth for about 90 minutes.

Scientists found that the geography and weather patterns on Saturn’s largest moon are somewhat similar to earth, though in place of breathable oxygen and a water cycle, the rivers and lakes of Titan are filled with methane. The “air” at its surface is a mixture of nitrogen and other elements that envelops the moon in a hazy atmosphere. 

Read Instride: Saturn


Mapping the Sky

January 31, 2017

In the 1920’s, the International Astronomical Union established the precise coordinates of the 88 constellations.

The most ancient constellations were observed more than 5,000 years ago, and they each tell a story about the civilization that first put into writing their view of the stars, the phases of the moon, and the seasonal changes that influenced their planting and harvesting.

Centuries later, the Greeks and then the Romans adapted these same star groupings to represent tales of love, hate, lust, and war among deadly creatures and legendary warriors. Relying solely on the sharpness of their eyesight, these early astronomers mapped the night sky with incredible accuracy.

When the first refracting telescopes were aimed at the stars in the 1700’s, new constellations were being “discovered” by explorers as they navigated the oceans near the North and South Pole, completing the map of the night sky.

Read Instride: History of the Constellations


Into the Storms of Jupiter

January 15, 2017

The Galileo probe’s 57 minute descent into Jupiter’s atmosphere in 1995 revealed that the planet is 90% hydrogen. In 2003, the orbiter dropped at speeds of 3000 km/m, sending temperature readings before being crushed by the heat and pressure.  

With the Juno orbiter, NASA scientists will spend the next two years gathering information about Jupiter’s gravity, magnetism, and atmosphere to determine whether the planet has a terrestrial core deep beneath raging storms of hydrogen and helium.

Read Instride: Jupiter

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The Ice Giants

January 5, 2017

When Voyager 2 (1977 – approx. 2025) completed its mission exploring Jupiter and Saturn, NASA scientists re-tasked the spacecraft to continue on, stopping at both Uranus and Neptune before traveling beyond the heliosphere. Though the ice giants have since been studied in depth by ground-based observatories, Voyager 2 is the only spacecraft to ever visit the outer planets.

Voyager 2 arrived at Uranus in 1986 after a five-year journey and surprisingly found that the third largest planet in the solar system was tipped on its side. Ten new satellites were discovered as well as a ring system. In contrast to the icy rings of Saturn, scientists theorize that the ones around Uranus consist of rock and metal and were formed by the collision of asteroids or a small moon. 

With a gravity assist from Uranus, Voyager continued on for another three years to Neptune. Five new moons and a sparse ring system were discovered. As with Uranus, the atmosphere of Neptune was believed to contain high levels of methane, causing the planets to appear blue-green. Voyager relayed information about the magnetic field of Neptune and the levels of solar radiation that exist 4.5 billion kilometers from the sun.

Read Instride: The Ice Giants