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Incoming! We’ve Got Science from Jupiter!

Our Juno spacecraft has just released some exciting new science from its first close flyby of Jupiter! 

In case you don’t know, the Juno spacecraft entered orbit around the gas giant on July 4, 2016…about a year ago. Since then, it has been collecting data and images from this unique vantage point.

Juno is in a polar orbit around Jupiter, which means that the majority of each orbit is spent well away from the gas giant. But once every 53 days its trajectory approaches Jupiter from above its north pole, where it begins a close two-hour transit flying north to south with its eight science instruments collecting data and its JunoCam camera snapping pictures.

Space Fact: The download of six megabytes of data collected during the two-hour transit can take one-and-a-half days!

Juno and her cloud-piercing science instruments are helping us get a better understanding of the processes happening on Jupiter. These new results portray the planet as a complex, gigantic, turbulent world that we still need to study and unravel its mysteries.

So what did this first science flyby tell us? Let’s break it down…

1. Tumultuous Cyclones

Juno’s imager, JunoCam, has showed us that both of Jupiter’s poles are covered in tumultuous cyclones and anticyclone storms, densely clustered and rubbing together. Some of these storms as large as Earth!

These storms are still puzzling. We’re still not exactly sure how they formed or how they interact with each other. Future close flybys will help us better understand these mysterious cyclones. 

Seen above, waves of clouds (at 37.8 degrees latitude) dominate this three-dimensional Jovian cloudscape. JunoCam obtained this enhanced-color picture on May 19, 2017, at 5:50 UTC from an altitude of 5,500 miles (8,900 kilometers). Details as small as 4 miles (6 kilometers) across can be identified in this image.

An even closer view of the same image shows small bright high clouds that are about 16 miles (25 kilometers) across and in some areas appear to form “squall lines” (a narrow band of high winds and storms associated with a cold front). On Jupiter, clouds this high are almost certainly comprised of water and/or ammonia ice.

2. Jupiter’s Atmosphere

Juno’s Microwave Radiometer is an instrument that samples the thermal microwave radiation from Jupiter’s atmosphere from the tops of the ammonia clouds to deep within its atmosphere.

Data from this instrument suggest that the ammonia is quite variable and continues to increase as far down as we can see with MWR, which is a few hundred kilometers. In the cut-out image below, orange signifies high ammonia abundance and blue signifies low ammonia abundance. Jupiter appears to have a band around its equator high in ammonia abundance, with a column shown in orange.

Why does this ammonia matter? Well, ammonia is a good tracer of other relatively rare gases and fluids in the atmosphere…like water. Understanding the relative abundances of these materials helps us have a better idea of how and when Jupiter formed in the early solar system.

This instrument has also given us more information about Jupiter’s iconic belts and zones. Data suggest that the belt near Jupiter’s equator penetrates all the way down, while the belts and zones at other latitudes seem to evolve to other structures.

3. Stronger-Than-Expected Magnetic Field

Prior to Juno, it was known that Jupiter had the most intense magnetic field in the solar system…but measurements from Juno’s magnetometer investigation (MAG) indicate that the gas giant’s magnetic field is even stronger than models expected, and more irregular in shape.

At 7.766 Gauss, it is about 10 times stronger than the strongest magnetic field found on Earth! What is Gauss? Magnetic field strengths are measured in units called Gauss or Teslas. A magnetic field with a strength of 10,000 Gauss also has a strength of 1 Tesla.  

Juno is giving us a unique view of the magnetic field close to Jupiter that we’ve never had before. For example, data from the spacecraft (displayed in the graphic above) suggests that the planet’s magnetic field is “lumpy”, meaning its stronger in some places and weaker in others. This uneven distribution suggests that the field might be generated by dynamo action (where the motion of electrically conducting fluid creates a self-sustaining magnetic field) closer to the surface, above the layer of metallic hydrogen. Juno’s orbital track is illustrated with the black curve. 

4. Sounds of Jupiter

Juno also observed plasma wave signals from Jupiter’s ionosphere. This movie shows results from Juno’s radio wave detector that were recorded while it passed close to Jupiter. Waves in the plasma (the charged gas) in the upper atmosphere of Jupiter have different frequencies that depend on the types of ions present, and their densities. 

Mapping out these ions in the jovian system helps us understand how the upper atmosphere works including the aurora. Beyond the visual representation of the data, the data have been made into sounds where the frequencies and playback speed have been shifted to be audible to human ears.

5. Jovian “Southern Lights”

The complexity and richness of Jupiter’s “southern lights” (also known as auroras) are on display in this animation of false-color maps from our Juno spacecraft. Auroras result when energetic electrons from the magnetosphere crash into the molecular hydrogen in the Jovian upper atmosphere. The data for this animation were obtained by Juno’s Ultraviolet Spectrograph. 

During Juno’s next flyby on July 11, the spacecraft will fly directly over one of the most iconic features in the entire solar system – one that every school kid knows – Jupiter’s Great Red Spot! If anybody is going to get to the bottom of what is going on below those mammoth swirling crimson cloud tops, it’s Juno.

Stay updated on all things Juno and Jupiter by following along on social media: Twitter | Facebook | YouTube | Tumblr

Learn more about the Juno spacecraft and its mission at Jupiter HERE.

Discovery challenges belief about brain’s cellular makeup

A discovery made by Junhwan Kim, PhD, assistant professor at The Feinstein Institute for Medical Research, is challenging science’s longstanding beliefs regarding the cellular makeup of the brain. This breakthrough was outlined in a study published in the journal Molecular and Cellular Biochemistry. Having a full understanding of the brain can help identify new therapies as well as develop guidelines to maintain brain health.

It has long been a belief in the scientific field that the building blocks of brain cells, phospholipids, are enriched by polyunsaturated fatty acids. When trying to prove that the brain, like other major organs, are made of polyunsaturated fatty acids, Dr. Kim and his team were surprised by the results.

“We found the opposite of what science has widely believed – phospholipids containing polyunsaturated fatty acids in the brain are lower than other major organs,” said Dr. Kim. “Knowing that there are lower amounts of polyunsaturated fatty acids in the brain, we may need to rethink how this acid impacts brain health and conditions like oxygen deprivation.”

Dr. Kim and his team analyzed brain, heart, liver and kidney tissue from animals and found that only 60 percent of the brain’s phospholipids were made up of polyunsaturated fatty acids. That’s compared to other organs, where the polyunsaturated fatty acid content is about 90 percent. It has also been previously presumed that high polyunsaturated fatty acids levels in the brain were what made it susceptible to oxygen deprivation or brain injury. Further research is required to find out the reasoning for the difference in acid levels, but it could also challenge beliefs about polyunsaturated fatty acids’ impact on these conditions.

“Dr. Kim’s findings challenge basic assumptions about the brain,” said Kevin J. Tracey, MD, president and CEO of the Feinstein Institute. “This paper is an important step to defining a new research path.”

Never give up on someone with a mental illness. When “I” is replaced by “we”, illness becomes wellness.

Shannon L. Alder (via psych2go)

6 Reasons Why Smart People Cant Find Happiness

Happiness is the feeling of contentment and satisfaction that is craved by many but only achieved by some. Happiness is relative and subjective. But for many successful individuals, the presence of a great family life and a flourishing career is often not enough. On some occasions these do not prevent an smart individual from feeling a sense of loneliness, often sadness and melancholy.

Here are six psychological reasons why smart people have a harder time finding happiness.

1. Intelligent people over-analyze

Many individuals with high levels of intelligence often over think and analyze everything that occurs in their life and surroundings. While their ability to analyze things is a great asset, the constant analysis of everything often lead to frustrations especially when coming up with an undesired conclusion.

Being able to see through people’s intentions is a burden that most people don’t get to carry. Oftentimes, knowing how ugly the real world is like is……

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