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2006-07-20 22:33:09 · 13 answers · asked by Anonymous in Science & Mathematics Astronomy & Space

13 answers

Not with tech like this.
But perhaps in the future.
Jupiter's atmosphere is composed of ~90% hydrogen and ~10% helium by number of atoms. The atmosphere is ~75%/24% by mass; with ~1% of the mass accounted for by other substances - the interior contains denser materials such that the distribution is ~71%/24%/5%. The atmosphere contains trace amounts of methane, water vapor, ammonia, and "rock". There are also traces of carbon, ethane, hydrogen sulphide, neon, oxygen, phosphine, and sulphur. The outermost layer of the atmosphere contains crystals of frozen ammonia.

This atmospheric composition is very close to the composition of the solar nebula. Saturn has a similar composition, but Uranus and Neptune have much less hydrogen and helium.

Jupiter's upper atmosphere undergoes differential rotation, an effect first noticed by Giovanni Cassini (1690). The rotation of Jupiter's polar atmosphere is ~5 minutes longer than that of the equatorial atmosphere. In addition, bands of clouds of different latitudes, known as tropical regions flow in opposing directions on the prevailing winds. The interactions of these conflicting circulation patterns cause storms and turbulence. Wind speeds of 600 km/h are not uncommon.

The only spacecraft to have descended into Jupiter's atmosphere to take scientific measurements is the Galileo probe (see Galileo mission). It sent an atmospheric probe into Jupiter upon arrival in 1995, then itself entered Jupiter's atmosphere and burned up in 2003.

Planetary rings
Rings of Jupiter
Jupiter has a faint planetary ring system composed of smoke-like dust particles knocked from its moons by energetic meteor impacts. The innermost doughnut-shaped ring, called the halo, is almost as thick (20,000km) as it is wide (22,800km). This is followed by the thinnest and brightest main ring, which is made of dust from the satellites Adrastea and Metis. Metis orbits within its fluid Roche Limit with Jupiter, and objects not rigidly attached to it may freely fall away from it and into Jupiter's gravitational field. Two wide gossamer rings encircle the main ring, originating from Thebe and Amalthea. Finally, there is a distant and very faint outer ring circling Jupiter backwards—retrograde of its spin. It's not known for sure where the material for this outer ring comes from, but it may be captured interplanetary dust.

Magnetosphere
Jupiter has a very large and powerful magnetosphere. In fact, if one could see Jupiter's magnetic field from Earth, it would appear five times as large as the full moon in the sky despite being so much farther away. The magnetic field is generated by eddy currents in Jupiter's metallic hydrogen core. This magnetic field collects a large flux of particle radiation in Jupiter's radiation belts, as well as producing a dramatic gas torus and flux tube associated with Io. Jupiter's magnetosphere is the largest planetary structure in the solar system.

The Pioneer probes confirmed that Jupiter's enormous magnetic field is 10 times stronger than Earth's and contains 20,000 times as much energy. The sensitive instruments aboard found that the Jovian magnetic field's "north" magnetic pole is at the planet’s geographic south pole, with the axis of the magnetic field tilted 11 degrees from the Jovian rotation axis and offset from the center of Jupiter in a manner similar to the axis of the Earth's field. The Pioneers measured the bow shock of the Jovian magnetosphere to the width of 26 million kilometres (16 million miles), with the magnetic tail extending beyond Saturn’s orbit.

The data showed that the magnetic field fluctuates rapidly in size on the sunward side of Jupiter because of pressure variations in the solar wind, an effect studied in further detail by the two Voyager spacecraft. It was also discovered that streams of high-energy atomic particles are ejected from the Jovian magnetosphere and travel as far as the orbit of the Earth. Energetic protons were found and measured in the Jovian radiation belt and electric currents were detected flowing between Jupiter and some of its moons, particularly Io.
Exploration of Jupiter
A number of probes have visited Jupiter.

Pioneer flyby missions

Image of Jupiter by Pioneer 10.Pioneer 10 flew past Jupiter in December of 1973, followed by Pioneer 11 exactly one year later. Pioneer 10 made the first ever close up images of Jupiter, studied its atmosphere, and detected its magnetic field.

Voyager flyby missions
Voyager 1 flew by in March 1979 followed by Voyager 2 in July of the same year. The Voyagers vastly improved the understanding of the Galilean moons and discovered Jupiter's rings. They also took the first close up images of the planet's atmosphere.

Ulysses flyby mission
In February 1992, Ulysses solar probe performed a flyby of Jupiter at a distance of 450,000 km (6.3 Jovian radii). The flyby was required to attain a polar orbit around the Sun. The probe conducted studies on Jupiter's magnetosphere. Since there are no cameras onboard the probe, no images were taken. In February 2004, the probe came again in the vicinity of Jupiter. This time the distance was much greater, about 240 million km.
Galileo mission
So far the only spacecraft to orbit Jupiter is the Galileo orbiter, which went into orbit around Jupiter on December 7, 1995. It orbited the planet for over seven years and conducted multiple flybys of all of the Galilean moons and Amalthea. The spacecraft also witnessed the impact of Comet Shoemaker-Levy 9 into Jupiter as it approached the planet in 1994, giving a unique vantage point for this spectacular event. However, while the information gained about the Jovian system from the Galileo mission was extensive in its own right, its originally-designed capacity was limited by the failed deployment of its high-gain radio transmitting antenna.

An atmospheric probe was released from the spacecraft in July, 1995. The probe entered the planet's atmosphere in December 7, 1995. It parachuted through 150 km of the atmosphere, collecting data for 57.6 minutes, before being crushed by the extreme pressure to which it was subjected. It would have melted and vaporized shortly thereafter. The Galileo orbiter itself experienced a more rapid version of the same fate when it was deliberately steered into the planet on September 21, 2003 at a speed of over 50 km/s, in order to avoid any possibility of it crashing into and possibly contaminating Europa, one of the Jovian moons.

Cassini flyby mission
In 2000, the Cassini probe, en route to Saturn, flew by Jupiter and provided some of the highest-resolution images ever made of the planet.

Future probes
NASA is planning a mission to study Jupiter in detail from a polar orbit. Named Juno, the spacecraft is planned to launch by 2010.

Because of the possibility of a liquid ocean on Jupiter's moon Europa, there has been great interest to study the icy moons in detail. A mission proposed by NASA was dedicated to study them. The JIMO (Jupiter Icy Moons Orbiter) was expected to be launched sometime after 2012. However, the mission was deemed too ambitious and its funding was canceled.

In 2007, Jupiter will also be briefly visited by the New Horizons probe, en route to Pluto.

Life on Jupiter
It is considered highly unlikely that there is any life on Jupiter, as there is little to no water in the atmosphere and any possible solid surface deep within Jupiter would be under extraordinary pressures. However, in 1976, before the Voyager missions, Carl Sagan hypothesized (with Edwin E. Salpeter) that ammonia-based life could evolve in Jupiter's upper atmosphere. Sagan and Salpeter based this hypothesis on the ecology of terrestrial seas which have simple photosynthetic plankton at the top level, fish at lower levels feeding on these creatures, and marine predators which hunt the fish. The Jovian equivalents Sagan and Salpeter hypothesized were "sinkers", "floaters", and "hunters". The "sinkers" would be plankton-like organisms which fall through the atmosphere, existing just long enough that they can reproduce in the time they are kept afloat by convection. The "floaters" would be giant bags of gas functioning along the lines of hot air balloons, using their own metabolism (feeding off sunlight and free molecules) to keep their gas warm. The "hunters" would be almost squid-like creatures, using jets of gas to propel themselves into "floaters" and consume them.[8] These ideas are only speculation and have no supporting evidence.

Physical characteristics
Equatorial diameter 142,984 km [1]
(11.209 Earths)
Polar diameter 133,709 km
(10.517 Earths)
Oblateness 0.064 87
Surface area 6.14×1010 km2
(120.5 Earths)
Volume 1.431×1015 km3
(1321.3 Earths)
Mass 1.899×1027 kg
(317.8 Earths)
Mean density 1.326 g/cm3
Equatorial gravity 23.12 m/s2
(2.358 gee)
Escape velocity 59.54 km/s
Rotation period 0.413 538 021 d (9 h 55 min 29.685 s) 1
Rotation velocity 12.6 km/s = 45,300 km/h
(at the equator)
Axial tilt 3.13°
Right ascension
of North pole 268.05° (17 h 52 min 12 s)
Declination 64.49°
Albedo 0.52
Surface temp. min mean max
110 K 152 K N/A K

Adjective Jovian
Atmospheric characteristics
Atmospheric pressure 70 kPa
Hydrogen ~86%
Helium ~14%
Methane 0.1%
Water vapor 0.1%
Ammonia 0.02%
Ethane 0.0002%
Phosphine 0.0001%
Hydrogen sulfide <0.00010%

2006-07-20 23:07:34 · answer #1 · answered by PrAt 3 · 1 0

Not on Jupiter proper, because Jupiter is not a rocky planet as is Mercury, Venus, Earth & Mars. Any spacecraft looking to 'land' on Jupiter would never settle on solid land. (In fact, if Jupiter had been more massive it would have been a star in its on right.)
The MOONS of Jupiter are a worthy destination though! Hopefully by 2030!

2006-07-21 06:09:07 · answer #2 · answered by Dan The Man 2 · 0 0

No, there is no surface to land on. It's a big ball of gas. And, there are fierce radiation belts surrounding the planet, so that a human being would need to be encased in several feet of lead or similar material to safely reach the planet's cloud tops.

But, we might be able to land on some of the outer moons of Jupiter, the ones well outside the radiation belts.

2006-07-21 05:42:26 · answer #3 · answered by Mark V 4 · 0 0

Can't land- Jupiter, Saturn, Neptune, Uranus are all gas giants- essentially, chemically they're almost like huge balls of farts. Theres a theory that the core may be metallic hydrogen- theres no evidence to support this speculation but its good solid speculation. The gravity would be like 10,000 times that of earth, also- once you land, you'd be destroyed.

2006-07-21 06:07:21 · answer #4 · answered by Anonymous · 0 0

It does not take too long... and it is not all gas

The problem with landing on Jupiter would be its terrible gravity that would crush us long before we got anywhere near something we could land on.

It is a huge planet with storms raging ..... but gravity is the killer

2006-07-21 05:40:00 · answer #5 · answered by blind_chameleon 5 · 0 0

I do believe that we will eventually, I believe that the next big step will be for people to travel to Mars, but I believe that we will eventually explore all of the other planets and even go beyond out solar system by the end of this century.

2006-07-21 05:42:34 · answer #6 · answered by Anonymous · 0 0

If when you say "land" you mean visit, I would say yes. We have dropped probes down into the Jovian atmosphere. A better question is when will we land on Europa.

2006-07-21 05:58:42 · answer #7 · answered by zippo 3 · 0 0

LOL!! They can't even get to fuccking Mars, I doubt Jupiter is anywhere in the near future!!!! =)

2006-07-21 06:09:50 · answer #8 · answered by Marilyn Monroe 2 · 0 0

I think it is not possible,Because,Due to it' heavy weight it has more gravity it causes problem while landing.So it is difficult to land.

2006-07-21 06:01:01 · answer #9 · answered by sena 2 · 0 0

No takes too long too get there.

2006-07-21 05:37:08 · answer #10 · answered by christyxy777777 5 · 0 0

WAST OF TIME I HAVE BEEN THERE NOT MUCH TO SEE

2006-07-21 05:39:27 · answer #11 · answered by Anonymous · 0 0

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