July 4 2016 Juno Arrival at Jupiter and
First Day of Spring for Mars Rovers Curiosity and Opportunity!
On July 4, 2016, NASA's Juno spacecraft arrives at planet Jupiter. That same day marks the start of Spring in Mars' southern hemisphere (spring equinox), where Mars rovers Curiosity and Opportunity are exploring.
So, what is spring like on Jupiter and Mars? Song lyrics may be all about romance, but spring is extreme on these two other worlds!
Mars orbiters salute the Juno mission as it reaches Jupiter on July 4, 2016.
Someday in the future, humans living on Mars might pull out a telescope and peer through it to see Jupiter and its moons. Until then, Mars orbiters are some of our best robot astronomers. Picture of Jupiter picture from Mars Reconnaissance Orbiter’s HiRISE camera on 1/31/07 (1); Picture of Jupiter and its moons imaged by Mars Global Surveyor’s Mars Orbital Camera on 5/22/03 (2).
Springtime on Jupiter lasts three Earth years. Seasons are longer on Jupiter because it takes about 12 Earth years to orbit the Sun. Even though spring is long, you'd have to be very close to the north or south pole to notice much of a difference between Jupiter's seasons.
That's because Jupiter's equator is inclined only a very small 3 degrees from the plane of its orbit around the Sun. So, a spring day on Jupiter is pretty much like all the rest. That's different from Earth and Mars, which tilt on their axes by about 23.5 and 25 degrees respectively.
So, what is spring like on Jupiter? Within the visible top of Jupiter's clouds, there's no relief from Jupiter's strong winds. They routinely blow at speeds greater than Earth's most powerful storms. Beneath the clouds, the winds are even more ferocious, clocked at 380 miles per hour.
Jupiter has less lightning than our home planet, but any springtime lightning on Jupiter would be hundreds of times more powerful than a lightning bolt on Earth.
Colorful clouds of water, ammonia, and sulfur compounds brighten the spring sky just as they do the rest of Jupiter's year.
Mars has four seasons just like Earth, but they last about twice as long. That's because it takes about two Earth years for Mars to go around the sun. July 4, 2016 just happens to be the first day of spring in the southern hemisphere on Mars, where Mars rovers Curiosity and Opportunity are exploring.
The southern hemisphere of Mars has a warmer, shorter spring and summer than in the north, as Mars is closest to the Sun towards the end of southern spring. Southern winter is longer, and the seasonal south polar cap is more extensive. That's because Mars is farthest away from the Sun then, moving more slowly in its elliptical orbit around the Sun. We don't notice such differences on Earth, because our planet has a near circular orbit. Going from a colder winter to a warmer spring can be quite dramatic.
For Opportunity, spring always comes as a welcome relief!
Sometimes, dust devils even lift dust off of rover solar panels! More dust equals less sun and reduced power for operations, so we like to see clean panels! Even if no dust devils arrive to lift dust from its solar panels, the sun is at a higher angle. That charges the rover's battery so it can explore more, avoid "naps," and even do some work at night!
Spring on Mars also brings a lot of weird changes to the polar caps!
Martian polar caps have a lot of carbon-dioxide (dry) ice. During the polar night, as much as a quarter of the atmosphere, which is also largely carbon dioxide, is lost to the surface as frost and snow. Imagine your barometer recording a 25% change in surface pressure as the seasons change! As Mars emerges from winter, warmer spring temperatures can have a big effect. When it's spring in either hemisphere the polar cap thaws and grows smaller. Because the atmosphere is so thin, the carbon-dioxide ice skips becoming a liquid, and goes straight to becoming a gas.
As the carbon dioxide ice turns into a gas, pressure builds up under the thinning, cracking ice. The gas can burst up, sending dust from below flying and swirling. The dust settles in all kinds of dramatic patterns, from starbursts to spiders! The ground can also collapse in patterns called “swiss cheese” terrain, where a thin layer of carbon-dioxide ice partially covers a water ice block below.