In Space Blog 2017-09-12T10:50:20+00:00

Its hurricane season, and a dangerous one, with as many as three or four storm systems that could potentially reach hurricane strength in the warm waters of the Atlantic Ocean. Hurricane Harvey made landfall in South Texas as a Category 4 on August 30-31. Hurricane Irma is a category 5 storm that was spinning across Puerto Rico and Cuba before making its way up the Florida coast. And the National Hurricane Watch Center at NOAA is keeping their “eye” on Hurricanes Katia and Jose as well.

Storm systems are formed when warm air rises and clashes with cold air, resulting in precipitation and heavy winds. Hurricanes and Tornadoes are made of the same elements of air and water as regular thunderstorms, but they have the potential to quickly grow in size and build up a rotational velocity that causes catastrophic destruction.

Hurricanes and Tornadoes spin simply because the earth is spinning. Meteorologists explain that a phenomenon called the Coriolis Effect causes wind and precipitation to arc toward the right in the northern hemisphere, creating storms that rotate in a counter-clockwise direction, and toward the left in the southern hemisphere, resulting in storms that spin clockwise.

Tornado alley” in the mid-western United States sees more tornado activity than any other country in the world. Cold air from the Rocky Mountains collides with warm air from the Gulf of Mexico, and winds begin to spin unpredictably. Wind direction within a tornado spins chaotically both in a circular direction and vertically. High in the sky, they’re usually connected to a dangerous cumulonimbus cloud while they touch down on earth, sweeping up anything in a pathway of destruction that could measure up to two miles wide and many miles long. Tornado alerts sound in regions where storm activity is likely, but a tornado isn’t classified until after it dissipates, allowing scientists to observe the damage it caused and place it on a scale ranging from F0-F5.

Hurricanes, in contrast, form in the ocean during the summer and early autumn. They gather speed as warm water evaporates and rises, clashing with cold air higher up in the atmosphere. As the water cools, condensation begins to form, creating torrential rainfall that contributes to coastal flooding as powerful storm surges flow inland. Hurricane winds mostly blow horizontally, and for this reason “hurricane hunters” have been known to safely fly a plane through the center of the storm, dropping instruments into the winds to measure speed and precipitation.

[ Read Instride: Tips and Checklists when a storm is heading your way ]

Extremes on Planet Earth

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

Mars Rocks!

When meteorites from space are found on earth, scientists can usually determine where they came from based on information about the 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. 

Read Instride: Mars

Solar system and Space Blog image of astronauts on Mars.

Deep Space Network

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 Earth

Solar system and Space Blog image of Deep Space Network

Mercury's Elliptical Orbit

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

Solar system and Space Blog image of elliptical orbits of Mercury and Venus

Earth's Moon

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 pole.

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: The Earth