Jupiter's Atmosphere: Questions & Answers

  • Thread starter Thread starter argonurbawono
  • Start date Start date
  • Tags Tags
    Atmosphere
AI Thread Summary
Jupiter's atmosphere exhibits varying wind speeds, creating distinct bands due to the planet's rapid rotation and the Coriolis effect, which causes winds to bend rather than move uniformly. The turbulence patterns observed are a result of convective heat transfer, similar to processes on Earth, where warm air rises and cool air fills the void. The immense size of Jupiter allows for larger turbulence patterns, which do not break into smaller curls due to the planet's thick atmosphere and high viscosity. The similarities between Earth's and Jupiter's atmospheric dynamics highlight fundamental principles of fluid motion. Understanding these concepts can clarify the behavior of gases in both planetary atmospheres.
argonurbawono
Messages
18
Reaction score
0
once i looked at short video clip of Jupiter atmosphere. i have questions in mind:
1. why the atmosphere seems to travel at different speed making up a number of sliding rings?why don't they travel together?
2. what makes the pattern of turbulence so huge? i think we need such an incredible viscousity to produce such an effect. why don't they break up into tiny curls?

i never learn astronomy, so please excuse my silly questions if they sound very trivial.
 
Astronomy news on Phys.org
Good questions. Let me reframe the issue slightly:

First, what is wind and how does it work on Earth? Wind is nothing more than convective heat transfer: warm air rises, cool air moves into take its place. Since it is warmer at the equator than the poles, the convection takes heat up and away from the equator and sends it to the poles. Now you may notice that winds around where you live often go in the same direction. So what causes that? That's the coriolis effect. If wind moves in a straight line while the Earth is rotating under it, that causes the wind to bend.

This first link has a good description of the coriolis effect, the second has a good diagram showing the prevailing wind directions:
http://www.rcn27.dial.pipex.com/cloudsrus/wind.html
http://seis.natsci.csulb.edu/rbehl/winds.htm

And here is a great link showing the two circulation patterns side-by-side:
http://www.classzone.com/books/earth_science/terc/content/investigations/es2704/es2704page02.cfm

Notice how similar the bands look to how wind circulates on Jupiter?! The names are different, but they match up almost exactly!
 
Last edited by a moderator:
wow... I've checked it.
so Earth atmosphere is actually just doing the same thing ...
 
Yep, but our atmosphere is thin and transparent, so we don't see it. :)
 
TL;DR Summary: In 3 years, the Square Kilometre Array (SKA) telescope (or rather, a system of telescopes) should be put into operation. In case of failure to detect alien signals, it will further expand the radius of the so-called silence (or rather, radio silence) of the Universe. Is there any sense in this or is blissful ignorance better? In 3 years, the Square Kilometre Array (SKA) telescope (or rather, a system of telescopes) should be put into operation. In case of failure to detect...
Thread 'Could gamma-ray bursts have an intragalactic origin?'
This is indirectly evidenced by a map of the distribution of gamma-ray bursts in the night sky, made in the form of an elongated globe. And also the weakening of gamma radiation by the disk and the center of the Milky Way, which leads to anisotropy in the possibilities of observing gamma-ray bursts. My line of reasoning is as follows: 1. Gamma radiation should be absorbed to some extent by dust and other components of the interstellar medium. As a result, with an extragalactic origin, fewer...
Both have short pulses of emission and a wide spectral bandwidth, covering a wide variety of frequencies: "Fast Radio Bursts (FRBs) are detected over a wide range of radio frequencies, including frequencies around 1400 MHz, but have also been detected at lower frequencies, particularly in the 400–800 MHz range. Russian astronomers recently detected a powerful burst at 111 MHz, expanding our understanding of the FRB range. Frequency Ranges: 1400 MHz: Many of the known FRBs have been detected...
Back
Top