Discovery of Jupiter

Voyager at Jupiter. image credit: NASA/JPL

No one can definitively say when the discovery of Jupiter took place nor who discovered it. Why is it so hard? It is one of the five planets that can be seen in the night sky. Only Venus and the Moon are brighter. Frankly, it is nearly impossible to miss. NASA lists the planet as having been discovered by the Ancients. The planet is called Marduk in ancient Babylonian texts, Zeus in early Greek manuscripts, and Jupiter in Roman antiquity.

What is known are some of the firsts in the exploration of Jupiter. In 1610, Galileo Galilei turned his rudimentary telescope on Jupiter, and realized that it had 4 large moons orbiting it: Io, Europa, Ganymede and Callisto. This was an important discovery, because it demonstrated that Earth was not the center of the Universe as proponents of the geocentric view believed.

In the1660s, Giovanni Cassini used his telescope to discover spots and bands across the surface of Jupiter, and was able to estimate the planet’s rotational period. He is thought to be the first to observe the planet’s Great Red Spot, a giant storm that is still raging. Imagine a single storm that rages for over 450 years and is larger than the Earth.

The first spacecraft to visit Jupiter up close was NASA’s Pioneer 10 in 1973. That mission was closely followed by Pioneer 11 in 1974. Both of NASA’s Voyager spacecraft flew past in 1979, sending back many of the famous pictures we’re all familiar with. Since then, the Ulysses solar probe, NASA’s Cassini spacecraft and New Horizons have all made flybys of the planet.

The only spacecraft to actually orbit Jupiter was NASA’s Galileo mission, which went into orbit in 1995. NASA scientists were not satisfied with a few orbits of Jupiter. They wanted to see a bit more of the Jovian system, so Galileo was sent to observe a few moons. Galileo is credited as being the first spacecraft to observe a comet hitting a planet(Jupiter), first to flyby an asteroid, first to discover an asteroid with a moon, and it was the first to measure the crushing atmospheric pressure of Jupiter with a descent probe. The mission discovered evidence of subsurface saltwater on Europa, Ganymede and Callisto and revealed the intensity of the volcanic activity on Io.

We may not know the exact date of the discovery of Jupiter, but we know many first about the planet. Even now, scientists are planning the next mission and hoping to be the first to discover something about the Jovian system.

Here are some images of the Jupiter flyby from NASA’s New Horizons spacecraft, and an article about Cassini’s flyby of Jupiter.

Here’s the archived page for NASA’s Galileo mission to Jupiter, and information about the Voyager mission’s images of Jupiter.

We’ve also recorded an entire show just on Jupiter for Astronomy Cast. Listen to it here, Episode 56: Jupiter, and Episode 57: Jupiter’s Moons.

Sources:
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter&Display=Facts
http://solarsystem.nasa.gov/galileo/

Mass of Jupiter

Jupiter and its moons. Image credit: NASA/JPL

The mass of Jupiter is 1.9 x 1027 kg. It is hard to fully understand a number that large, so here are a few comparisons to help. It would take 318 times Earth’s mass to equal Jupiter’s. Jupiter is 2.5 times more massive than all of the other planets in our Solar System combined. Jupiter is actually so massive that if it gained much more mass it would shrink.

How can additional mass cause a planet to shrink? Gravitational compression. Given that there is no more hydrogen or helium gas floating around for Jupiter to collect, it would gain mass through the accretion of rocky bodies like asteroids. Jupiter’s intense gravity would pull additional rock tightly together shrinking the diameter of the planet and increasing its density. As the density increased so would the gravity, further compressing the planet. Scientists estimate that Jupiter would have to accumulate 3-4 times its current mass in order to begin compressing. Since there isn’t that much material in our Solar System, it is a pretty good bet that Jupiter will never shrink.

But what if it did? There have been rumors floating around for decades that Jupiter could ignite fusion and become a star at any time. They are all false science and garbage at best. The mass of Jupiter is no where near enough for sustained nuclear fusion. Fusion requires high temperatures, intense gravitational compression, and fuel. Jupiter has the right fuels in abundance. There is plenty of hydrogen to be had, but the planet is too cold and lacks the density for a sustained reaction process. Scientists estimate that Jupiter needs 50-80 times its current mass to ignite fusion. As stated in the paragraph above, there isn’t enough material to be had, so Jupiter can not become a star.

At one time, scientists thought that Jupiter was the largest that a planet could become without igniting fusion and becoming a star. They discovered the fallacy of that belief once technology expanded their view of the universe. According to Dr. Sean Raymond, a post doctoral researcher at the Center for Astrophysics and Space Astronomy (CASA) at the University of Colorado, ”In terms of gaseous planets, once they reach 15 Jupiter masses or so there is enough pressure in the core to ignite deuterium fusion, so those are considered ‘brown dwarfs’ rather than planets.”

As you can see, the mass of Jupiter may seem awesome in comparison to Earth, it is a tiny fish in a world of sharks. Scientists have found a few hundred gas giants larger than Jupiter as they have surveyed the night sky. Who knows what is in store as telescope technology improves in the coming years.

Here’s an article from Universe Today explaining just how big planets can get, and an article about how Jupiter and the other gas giants might have gobbled up their moons while they were forming.

This site has more detailed information about the mass of Jupiter, and a page from NASA that helps you calculate the density of the planets.

We’ve also recorded an entire show just on Jupiter for Astronomy Cast. Listen to it here, Episode 56: Jupiter, and Episode 57: Jupiter’s Moons.

Sources:
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter
http://planetquest.jpl.nasa.gov/news/tres4.cfm

Just in Time for Summer: The Milky Way Loses Weight

The Milky Way and its dark matter halo. Image credit: Sloan Digital Sky Survey

Have you ever been surprised at your annual weigh-in at the doctor’s office to find that your bathroom scale at home was wrong? Or, bought a new scale that had a difference of opinion with your old one? That’s what has happened with our very own Galaxy, the Milky Way. “The Galaxy is slimmer than we thought,” said Xiangxiang Xue of the Max Planck Institute for Astronomy in Germany and the National Astronomical Observatories of China, who lead a research team using the Sloan Digital Survey to measure the mass of the stars in the galaxy. “We were quite surprised by this result,” said Donald Schneider, a member of the research team, from Penn State. The researchers explained that it wasn’t a Galactic diet that accounted for the galaxy’s recent slimming, but a more accurate scale.

The researchers used the motions of distant stars to make the new determination of the Milky Way’s mass. They measured the motions of 2,400 “blue horizontal branch” stars in the extended stellar halo that surrounds the disk of the galaxy. These measurements reach distances of nearly 200,000 light years from the Galactic center, roughly the edge of the region illustrated in the image above. Our Sun lies about 25,000 light years from the center of the Galaxy, roughly halfway out in the Galactic disk. From the speeds of these stars, the researchers were able to estimate much better the mass of the Milky Way’s dark-matter halo, which they found to be much ‘slimmer’ than thought before.

The discovery is based on data from the project known as SEGUE (Sloan Extension for Galactic Understanding and Exploration), an enormous survey of stars in the Milky Way. Using SEGUE measurements of stellar velocities in the outer Milky Way, a region known as the stellar halo, the researchers determined the mass of the Galaxy by inferring the amount of gravity required to keep the stars in orbit. Some of that gravity comes from the Milky Way stars themselves, but most of it comes the distribution of invisible dark matter, which is still not fully understood.

The most recent previous studies of the mass of the Milky Way used mixed samples of 50 to 500 objects. They implied masses up to two-trillion times the mass of the Sun for the total mass of the Galaxy. By contrast, when the SDSS-II measurement within 180,000 light years is corrected to a total-mass measurement, it yields a value slightly under one-trillion times the mass of the Sun.

“The enormous size of SEGUE gives us a huge statistical advantage,” said Hans-Walter Rix, director of the Max Planck Institute for Astronomy. “We can select a uniform set of tracers, and the large sample of stars allows us to calibrate our method against realistic computer simulations of the Galaxy.” Another collaborator, Timothy Beers of Michigan State University, explained, “The total mass of the Galaxy is hard to measure because we’re stuck in the middle of it. But it is the single most fundamental number we have to know if we want to understand how the Milky Way formed or to compare it to distant galaxies that we see from the outside.”

All SDSS-II observations are made from the 2.5-meter telescope at Apache Point Observatory in New Mexico. The telescope uses a mosaic digital camera to image large areas of sky and spectrographs fed by 640 optical fibers to measure light from individual stars, galaxies, and quasars. SEGUE’s stellar spectra turn flat sky maps into multi-dimensional views of the Milky Way, Beers said, by providing distances, velocities, and chemical compositions of hundreds of thousands of stars.

Source: Penn State, arXiv

Interview in Australia Today (or is it tomorrow?)

Update: Well, I guess it will be tomorrow! Due to some technical difficulties with phones, we weren’t able to do the interview today, so will try again tomorrow, same time. Keeping fingers crossed it works then.

I (Nancy) will be doing a live interview on an Australian radio show called “The Starlight Zone” with Col Maybury of radio station 2NUR FM, a community radio station funded and operated by the University of Newcastle. For me, the interview will be on Wednesday Thursday at 3:50 pm (US Central Time) but in Australia it will actually be Thursday Friday morning at 6:50 am! How confusing! To keep it simple, the time is 20:50 Universal Time.

You can listen live HERE, (Look for the link on the left that says “Listen”) but I believe a recording will also be available later, and if so I’ll post it here at that time.

The interview will only be 5 minutes long, and from what Col has told me, he wants to ask me about the concept of a one-way mission to Mars (or maybe this one).

Hope you can listen in.

Is There Life on Jupiter?

As an avid reader, I have come across many books that proposed the idea of life on Jupiter. Some even proposed that Jupiter is lifeless, but its moons harbor advanced life forms. Is there life on Jupiter? While there have been no samples taken that could test for microscopic life on the planet, there is quite a bit of compelling evidence that shows there is no possible way for life as we know it to exist anywhere on the planet. Try this link for one scientist’s take on finding life in the cosmos.

First, let’s look at the conditions on Jupiter that preclude the existence of life. The planet is a gas giant composed mainly of hydrogen and helium. There is virtually no water to support known life forms. The planet does not have a solid surface for life to develop anywhere except as a floating microscopic organism.

Free floating organisms could only exist at the very tops of the clouds due to atmospheric pressure that is progressively more intense than anything seen on Earth. While the cloud tops could harbor life that is resistant to solar radiation, the atmosphere is in constant chaos. Convection forces the lower atmosphere upwards and colder areas of the atmosphere are constantly being sucked closer to the core. The churning would eventually expose any organisms to the extreme pressures nearer the core, thus killing any that may develop.

Should an organism find a way to resist atmospheric pressure that reaches 1,000 times what it is here on Earth, there are the temperatures close to the planet’s core. Gravitational compression has heated areas near the core to over 10,000 degrees Celsius. It is so hot in some areas that hydrogen is in a liquid metallic state. While organisms on Earth live in areas near volcanoes, the temperatures there do not approach Jovian levels.

Jupiter is completely inhospitable to life as we understand it, but its moon Europa has been proposed as a possible habitable zone. It is thought to have a large amount of water ice on its surface. Some of which covers a proposed ocean of water slush. The conditions under the water ice could be harboring microscopic life according to some scientists.

The question ”is there life on Jupiter” seems pretty well decided. There is no way that life as we understand it could exist on the gas giant. The possibility of life within the Jovian system is still being explored. Some debate exists about Europa. NASA’s Jupiter Icy Moons Orbiter was set to answer those questions before it was canceled. Hopefully, another mission like it will be launched soon and end all of the debate.

Here’s an article about the search for life on Europa. Not so fast, though. Here’s an article about how Europa might be corrosive to life.

Here’s a classic article from Time Magazine in 1961 about the possibilities of life on Jupiter, and the search for life on Jupiter’s moon Europa.

We’ve also recorded an entire show just on Jupiter for Astronomy Cast. Listen to it here, Episode 56: Jupiter, and Episode 57: Jupiter’s Moons.

Sources:
http://www.nasa.gov/vision/universe/starsgalaxies/frozenworlds.html
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jup_Europa
NASA Jimo MIssion

New Lunar Prototype Vehicles Tested (Gallery)

NASA recently took some of its most promising new concepts for living and working on the moon and tried them out in a moon-like location near Lake Moses, Washington. Scout robots, rovers, cargo carriers, cranes and spacesuits endured sand storms and temperature swings to help test out the prototypes and prepare for future lunar expeditions. Although conditions on the moon will be much harsher, one investigator said, “It’s as close as we can get in a terrestrial environment to the lunar environment.” Above is the Mobile Lunar Transporter, which includes unique features that allow each of its six wheels to move independently, giving the vehicle the ability to drive in any direction. The human drivers stood in turrets on the “trucks.”

JPL tested two ATHLETE cargo-moving rovers they are developing. These rather odd-looking transport vehicles have legs capable of rolling or walking over extremely rough or steep terrain. They can carry, manipulate, deposit and transport payloads to desired sites. Maybe they’ll become the lunar version of a Winnebago, and future lunar astronauts can also take them out on weekend camping trips.

This Autonomous Drilling Rover could be used to search for valuable resources under the lunar surface in the moon’s polar regions. Its made to operate in extreme cold and dark conditions.

This lunar bulldozer, called LANCE (Lunar Attachment Node for Construction Excavation), is designed to be used with the lunar truck. The bulldozer can be used to help prepare a site for building an outpost on the moon.

These K10 scout robots can perform highly repetitive and long-duration tasks. During the tests, the rovers surveyed simulated lunar landing sites and built topographic and panoramic 3-D terrain models. One rover used a ground-penetrating radar to assess subsurface structures. The other used a 3-D scanning laser system known as LIDAR to create topographic maps. They can also perform science reconnaissance.

And of course, we can’t have humans on the moon without having spacesuits, so some of the new design of spacesuits were tested as well.

More info about these tests, which took place on June 2-13, 2008.

University Returns $3 Million in Savings to NASA

Here’s something you don’t read everyday: The University of Colorado at Boulder returned nearly $3 million in cost savings to NASA for the SORCE mission, the Solar Radiation and Climate Experiment, which studies how the sun’s variation influences Earth’s climate and atmosphere. The university designed, built and controls the mission. Tom Woods, principal investigator of SORCE said the cost savings were the result of a small, efficient management team, thorough pre-launch testing of prototype instruments and tight schedule adherence during the development phase. “We have a long history at LASP (Laboratory for Atmospheric and Space Physics, in Boulder) in mission and instrument development and spaceflight management and operations, and our experience clearly showed here,” said Woods. “We didn’t cut any corners, we made the best use of the available budget, and we are extremely pleased to be able to return this substantial cost savings back to NASA.”

The SORCE mission was launched by NASA in 2003. Its total budget of $100 million from 1999 to 2008 included the design and development of the satellite’s five instruments, as well as five-and-one-half years of operations, and did not include launch costs. A $2,997,000 check for the cost savings from SORCE development and operations was presented to NASA officials on June 17.

According to Woods, the cost savings during flight operations were largely due to the “sharing” of Laboratory for Atmospheric and Space Physics (LASP) personnel who also operate three other NASA satellites — ICEsat, QuikSCAT and AIM — from the CU Research Park in Boulder.
According to NASA, CU-Boulder is the single largest recipient of NASA university research dollars in the nation. In fiscal year 2007, CU-Boulder received $46.9 million from NASA and an additional $3 million in federal funds for space research from the Jet Propulsion Laboratory in Pasadena and the Space Telescope Science Institute in Baltimore.

SORCE is part of NASA’s Earth Observing System and has greatly expanded measurements of the sun’s radiation, covering wavelengths from soft x-ray bands and ultraviolet light through the visible and near-infrared wavelengths, said Woods. Accurate measurements of solar variation are essential for predicting the sun’s influence on climate and the atmosphere and quantifying how humans are changing the environment, he said.

The SORCE mission was recently extended through 2012, providing LASP with an additional $18 million for satellite operations and data analysis. NASA ranked the SORCE mission as excellent across the board for quality, timeliness, cost and leadership, a ranking achieved by only 4 percent of all NASA missions.

Original News Source: PhysOrg

Seals Use Astronomy as Navigation Aid

A baby Harp Seal, looking upward (Care2.com)

Yes, we’ve heard bees use the Earth’s magnetic field to navigate by. We’ve also heard about some bird species following the Sun to find the location of their evening roost. But what do we know about the animals living at sea? Do they use astronomical aids to help them find their way around the planet? Mammals such as whales are known to exhibit “skyhopping” behaviour when they surface from the water to have a look around, but seals go one step further; they can recognise and orientate themselves with the stars…

It was one of the first methods us humans used for navigation when sailing across the middle of a featureless ocean, we’d pick out known stars and constellations and relate them to our location on the planet’s surface. Explorers used astronomy to guide them to new lands, captains used the stars to direct their battleships toward the enemy and trade routes were repeatedly used thanks to star navigation. In its most basic form, star navigation could be carried out by linking stars with the location on the horizon when they rise, as was traditionally done by Polynesian sailors to colonize vast numbers of islands in the Pacific.

In a revealing study, researchers at the University of Southern Denmark in Odense have discovered that seals have the ability to recognise stars and groups of stars inside a modified planetarium. A five-metre round pool plus two harbour seals were covered with a dome with 6000 point light sources to simulate the Northern Hemisphere’s starry sky. Björn Mauck and his team found that if they selected an individual star with a laser pointer, they could train the seals to swim toward that star and then rewarded them with a treat if they did it correctly. Then the researchers would randomly orientate the dome, and without the help of a laser pointer, the seals would continue to swim toward the correct star.

Seals and many other animals are exposed to the starry sky every clear night, and thus certainly have sufficient opportunities to learn the patterns of stars.” – Björn Mauck

This study strongly suggests that these two harbour seals have an amazing, natural ability to recognise the distribution of stars on a clear night.

So when you next see a seal popping to the ocean surface, it might not be simply checking out its surroundings, it might be trying to look for Sirius in the constellation of Canis Major…

Paper abstract: “Harbour seals (Phoca vitulina) can steer by the stars“, Mauck et al., 2008
Source: New Scientist

Orbit of Jupiter

Orbit of the planets. Image credit: NASA/JPL

The orbit of Jupiter, like that of all the planets, is elliptical instead of circular. At perihelion(closest approach) Jupiter comes within 741 million km, or 4.95 astronomical units(AU), of the Sun. An astronomical unit is the average distance from the Earth to the Sun and is used to make astronomical distances easier to communicate. At its most distant point, called aphelion, Jupiter is 817 million km, or 5.46 AU from the Sun. The average between perihelion and aphelion is called the semi-major axis. Jupiter’s semi-major axis is 778 million km, or 5.2 AU.

Jupiter is the fifth planet from the Sun, but it is the third brightest object in the night sky here on Earth. Since Jupiter is farther from the Sun, you would expect it to take longer to orbit, but did you know that it takes 11.86 Earth years, or 4331 Earth days for Jupiter to complete one orbit? Jupiter travels at 47,002 km/h through ts orbit. Its orbit is inclined 6.09 degrees from the the Sun’s equator. Several of the planets have seasons, similar to Earth’s, but Jupiter does not. It rotates too fast for seasonal variations(Jupiter rotates every 10 hours).

Jupiter has several companions in its orbit. By companions, I mean moons. There are 64 known moons in orbit around Jupiter with a few more being suspected. The largest four(Io, Europa, Ganymede, and Callisto) are are called the Galilean satellites. They are diverse and interesting worlds of their own. Io is the most volcanically active body in our Solar System. Europa is covered in water ice which may be covering an ocean of slushy water. Ganymede is larger than Mercury and it is the only moon in the Solar System that generates its own magnetic field. Callisto’s surface is heavily cratered and some of the larger craters may have been in place shortly after the creation of the Solar System, yet some small craters show indications of recent geologic activity. Four of Jupiter’s moons are thought to be the source of its rings. Adrastea and Metis contribute to the main ring and the halo ring. Amalthea and Thebe contribute to two separate gossamer rings.

The orbit of Jupiter is beyond comparison in our Solar System. The Jovian influence can be felt well beyond its orbit. There is so much within that orbit that scientists can make an entire career out of studying the Jovian system.

Here’s an article on Universe Today about how Jupiter might have caught one of its moons while orbiting the Sun, and more detailed information about how long a year is on Jupiter.

Here’s Hubblesite’s News Releases about Jupiter, and more information on Jupiter in NASA’s Solar System Exploration pages.

We’ve also recorded an entire show just on Jupiter for Astronomy Cast. Listen to it here, Episode 56: Jupiter, and Episode 57: Jupiter’s Moons.

Source:
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter&Display=Facts

Does Jupiter Have Rings

Jupiter's rings. Image Credit: University of Maryland

We all known that Saturn has rings, but does Jupiter have rings? Yes, it does. Four planets have a rings system: Saturn, Jupiter, Uranus, and Neptune. Saturn is best know because it has the brightest and most extensive rings system in the Solar System.

The rings around Jupiter had never been seen before Voyager 1 arrived in 1979. Since then the rings have been observed by the largest telescopes on Earth, the Hubble Space Telescope, and the New Horizons spacecraft. So far, only four rings have been observed: the halo ring, the main ring, the Amalthea gossamer ring, and the Thebe gossamer ring.

Jupiter’s rings and moons exist within an intense radiation belt of electrons and ions trapped in the planet’s magnetic field. These particles and fields comprise the Jovian magnetosphere or magnetic environment, which extends 3 to 7 million km toward the sun, and stretches in a windsock shape at least 750 million km, which puts it inside of Saturn’s orbit.

The main ring is about 7,000 km wide and has an abrupt outer boundary 129,130 km from the center of the planet. The main ring encompasses the orbits of two small moons, Adrastea and Metis, which may act as the source for the dust that makes up most of the ring. The ring needs a constant source of dust because small particles can only exist for 100 to 1000 years. The dust is thought to rise from moons within the rings due to micrometeoroid impacts. The main ring merges gradually into the Halo ring. The halo is a broad, faint torus of material about 20,000 km thick and extending halfway from the main ring down to the planet’s cloudtops.

On the outer edge of the main ring and opposite of the halo ring, is the broad and extremely faint Amalthea gossamer ring. This ring extends out beyond the orbit of the moon Amalthea. Scientists believe that it is composed of dust particles smaller than 10 microns. 10 microns is about the size of cigarette smoke particles. It extends to an outer edge of about 129,000 km from the center of the planet and inward to about 30,000 km. The origin of the ring is probably from micrometeorite bombardment of the tiny moons orbiting within the ring. Last, is the Thebe gossamer ring. This is the faintest of the Jovian rings and extended from the orbit of the moon Thebe at about 226,000 km towards the planet, ending at about 129,000 km. The exact inner edges of the two gossamer rings are hard to define because they overlap the brighter main ring.

So, the answer to ”does Jupiter have rings” is yes, it has four known rings. Be sure to read about the ring systems of Neptune and Uranus as well.

Here’s a news article from Universe Today about the rings of Jupiter, and information about New Horizon’s observations of Jupiter’s rings.

Here’s NASA’s Solar System explorer information about Jupiter’s rings, and a cool image from Astronomy Picture of the Day of Jupiter’s rings.

We’ve also recorded an entire show just on Jupiter for Astronomy Cast. Listen to it here, Episode 56: Jupiter, and Episode 57: Jupiter’s Moons.

Source:
http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter&Display=Rings