Where In The Universe?

The past couple of weeks we’ve had a ‘mystery’ image, and asked our readers to guess what world in our solar system was featured in the image. Most everyone seemed to enjoy it, and it was fairly popular, so we’ve decided to make it a regular feature. I was going to call it the ‘Wednesday Where in the World (and What World) Is This?’ but that’s just too long, not to mention too many W’s in one headline. So to brief it up, and since this is “Universe Today,” we’ve decided to call it “Where In The Universe?” Look for it every Wednesday.

Above is this week’s mystery image. If you keep an eye on the images being released by the various spacecraft traveling our solar system, you may have seen this one before. Remember, you have 8 planets, 169 known moons, a handful of dwarf planets and lots of asteroids in our solar system to choose from. Don’t cheat — make your guess before you click to continue…

This is an image of Saturn’s moon Titan, taken by the Huygen’s probe as it descended through Titan’s thick atmosphere and down to the surface. It’s a Mercator projection, or a flattened image of the curved globe of Titan. Don’t feel bad if you guessed Mars — the coloring and mountains are reminiscent of Mars, or even some areas on Earth. It’s exciting to know that Titan has those similar features, too.


This is a full poster of images taken at four different altitudes from the descent imager/spectral radiometer on the European Space Agency’s Huygens probe, showing aerial views of the landing site. The images were taken on Jan. 14, 2005. Coming up in less than 12 days, Cassini will flyby Titan at a fairly close proximity, at about 1000 km (621 miles) above the surface of this interesting moon. The flyby will be on May 12, 2008.

Original Source: Cassini website

What Color is Mercury?

True color image of Mercury (MESSENGER)

Unlike all of the other planets in the Solar System, Mercury is just bare rock. It does have a tenuous atmosphere, but ground and space-based observations see just the gray rocky color of Mercury. This gray color comes from Mercury’s molten surface that cooled and hardened billions of years ago after the formation of the Solar System.

There are no active tectonic or erosion processes happening on the surface of Mercury; it has remained unchanged for billions of years, reshaped only by the occasional meteorite impact. In the past, some of the basins were filled in by magma that flowed out of the planet when it still had an active geologic cycle. Geologists are fairly certain that there are no active volcanoes on Mercury any more, but it’s possible that there could still be the occasional lava flow. Fresh lava flows would appear as a different color on the surface of Mercury. Perhaps when NASA’s MESSENGER spacecraft enters orbit around Mercury, we’ll get a better idea of its colors. Certainly we’ll know more about its surface geology.

The photograph attached to this article provides one of the best true-color images of Mercury that we have. If you could fly over Mercury in your spacecraft, this is essentially what you’d see. The planet Mercury color is a dark gray surface, broken up by craters large and small. The color of Mercury’s surface is just textures of gray, with the occasional lighter patch, such as the newly discovered formation of crater and trenches that planetary geologists have named “The Spider”.

Mercury’s coloring is very similar to the Earth’s moon. In fact, when you’re looking at images of both objects, it’s very difficult to tell the two objects apart. Unlike the Moon, however, Mercury lacks the darker areas, or “seas”, that were created on the Moon by lava flows. Mercury’s color doesn’t have the variety that even the Moon has.

If you got here not asking what color is Mercury the planet, but what color is Mercury (the element), it’s silver, and a liquid at room temperature.

We have written many stories about Mercury here on Universe Today. Here’s an article about a side of Mercury never before seen by spacecraft, and here’s a story about the color of Mercury captured by NASA’s MESSENGER spacecraft during a recent flyby.

If you’d like more information on Mercury, check out NASA’s Solar System Exploration Guide, and here’s a link to NASA’s MESSENGER Misson Page.

We have also recorded a whole episode of Astronomy Cast that’s just about planet Mercury. Listen to it here, Episode 49: Mercury.

Reference:
New Science Findings From Messenger’s Third Mercury Flyby
NASA Science: Surprises from Mercury
NASA Solar System Exploration

Titan Launch Pad Tower Blown Up at Cape Canaveral (Gallery)

The demolition of the old Titan pad gantry, photo sequence (Chris Miller/Spaceflight Now)

Cape Canaveral’s Titan launch pad gantry was demolished on Sunday. The tower was built in the 1990’s to support the US Air Force Titan 4 rocket program. The site has been used for NASA missions as well, including the launch of the Cassini-Huygens Saturn mission in 1997. Launch Complex 40 is being demolished and then refurbished to make way for the new SpaceX Falcon rocket launch facility. Now the gantry is rubble, the clean up operation can begin…

Debris of the launch gantry (Chris Miller/Spaceflight Now)

At 9am on Sunday, April 27th, 200 pounds of high explosives brought the Complex 40 mobile service tower crashing down. The tower was responsible for housing and preparing the highly successful Titan rockets for launch. Mainly used for military payloads, the Titan 4 series also sent the NASA Cassini probe on its way to Saturn on October 15th, 1997. A Titan 4 rocket was also used to send the ill-fated Mars Observer mission to the Red Planet on September 25th, 1992. Mission controllers lost contact with Observer when it was three days away from orbital insertion.

A Titan 4 rocket pre-launch as the gantry rolls back. The lightning protection system surrounds the pad (Justin Ray/Spaceflight Now)

The gantry weighed nearly 6500 tonnes and was installed with an advanced satellite processing clean room. The tower supported a total of 17 launches, deploying sophisticated surveillance and communication satellites for the US government. Two of these launches were devoted to the NASA interplanetary missions. The last Titan 4 was launched three years ago, handing heavy launch duties over to the modern Atlas 5 and Delta 4 rocket systems. In its glory days Titan 4 was the largest rocket available carrying the heaviest payloads into space.

View the complete series of images taken of the demolition of the Complex 40 tower »

Now that the tower has been removed, Space Exploration Technologies (SpaceX) can begin to set up the commercial launch site as the East Coast base of operations for its Falcon 9 rocket system which is currently under development. But why can’t the tower be renovated for SpaceX launches? The Falcon 9 rocket system will be assembled horizontally and rolled to the launch pad shortly before launch; the gantry is therefore superfluous to the company’s needs at Complex 40.

SpaceX Falcon 1 rocket system in 2004 (SpaceX)

However, not all the infrastructure of the site will be removed. The launch pad’s concrete deck and flame duct, water deluge system, electrical systems, lightning towers and instrumentation in the bay under the pad will be reused. The existing office space will also be renovated for SpaceX use. Since last October, SpaceX employees have been working at the site, removing any equipment not compatible with the Falcon system. The site will be up and running in time to begin supplying the International Space Station when NASA’s Space Shuttle fleet is retired in 2010. Complex 40 will live on, minus gantry, for NASA contracted launches and other commercial satellite orbital insertions by SpaceX.

Sources: SpaceX, Spaceflight Now

Cassini Watches Five-Month-Long Lightning Storm Rage on Saturn

Cassini scientists know for sure their spacecraft isn’t in Kansas anymore. Cassini’s been keeping an eye on a powerful electrical storm that’s been raging on Saturn for five months now, with lightning bolts 10,000 times more powerful than those found on Earth. But Cassini has also been busy flying by moons like Enceladus and Titan during this time, and therefore can’t constantly watch the storm. So amateur astronomers have been assisting the Cassini science team by monitoring this tempest in the “Storm Alley” region of Saturn. It’s no Great Red Spot, but it’s the longest lasting electrical storm ever detected in our solar system.

This prolonged storm is located in Saturn’s southern hemisphere–in a region nicknamed “Storm Alley” by mission scientists–where previous, but much shorter-lived lightning storms (if month-long storms can be called short!) were observed by Cassini. Saturn’s electrical storms are similar to thunderstorms on Earth, but they’re much bigger and longer lasting. Storms on Saturn have diameters of several thousand kilometers (thousands of miles), and radio signals produced by their lightning are thousands of times more powerful than those produced by terrestrial thunderstorms.

The storm was first detected on Saturn on Nov. 27, 2007. The electrostatic discharges were picked up by Cassini’s radio and plasma wave science instrument.

“The electrostatic radio outbursts have waxed and waned in intensity for five months now,” said Georg Fischer, an associate with the radio and plasma wave science team at the University of Iowa, Iowa City. “We saw similar storms in 2004 and 2006 that each lasted for nearly a month, but this storm is longer-lived by far. And it appeared after nearly two years during which we did not detect any electrical storm activity from Saturn.”

Amateur astronomers have kept track of the storm over its five-month lifetime. “Since Cassini’s camera cannot track the storm every day, the amateur data are invaluable,” said Fischer. “I am in continuous contact with astronomers from around the world.”

The long-lived storm will help provide information on the processes powering Saturn’s intense lightning activity. Cassini scientists will continue to monitor Storm Alley as the seasons change, bringing the onset of autumn to the planet’s southern hemisphere.

Original News Source: Cassini Press Release

Supermassive Black Hole Kicked Out of Galaxy: First Ever Observation

Colliding galaxies can force the supermassive black holes in their cores together (NCSA)

For the first time, the most extreme collision to occur in the cosmos has been observed. Galaxies are known to hide supermassive black holes in their cores, and should the galaxies collide, tidal forces will cause massive disruption to the stars orbiting around the galactic cores. If the cores are massive enough, the supermassive black holes may become trapped in gravitational attraction. Do the black holes merge to form a super-supermassive black hole? Do the two supermassive black holes spin, recoil and then blast away from each other? Well, it would seem both are possible, but astronomers now have observational evidence of a black hole being blasted away from its parent galaxy after colliding with a larger cousin.

Most galaxies in the observable universe contain supermassive black holes in their cores. We know they are hiding inside galactic nuclei as they have a huge gravitational dominance over that region of space, sucking away at stars orbiting too close. Recent observations of galactic cores show quickly rotating stars around something invisible. Calculating the star orbital velocities, it has been deduced that the invisible body they are orbiting is something very massive; a supermassive black hole of hundreds of millions of solar masses. They are also the source of bright quasars in active, young galaxies.

Now, the same research group who made the astounding discovery of the structure of a black hole molecular torus by analysing the emission of echoed light from an X-ray flare (originating from star matter falling into the supermassive black hole’s accretion disk) have observed one of these supermassive black holes being kicked out of its parent galaxy. What caused this incredible event? A collision with another, bigger supermassive black hole.

A cartoon of a superkick (MPE/HST)

Stefanie Komossa and her team from the Max Planck Institute for extraterrestrial Physics (MPE) made the discovery. This work, to be published in Astrophysical Journal Letters on May 10th, verifies something that has only been modelled in computer simulations. Models predict that as two fast-rotating black holes begin to merge, gravitational radiation is emitted through the colliding galaxies. As the waves are emitted mainly in one direction, the black holes are thought to recoil – much like the force that accompanies firing a rifle. The situation can also be thought of as two spinning tops, getting closer and closer until they meet. Due to their high angular momentum, the tops experience a “kick”, very quickly ejecting the tops in the opposite directions. This is essentially what two supermassive black holes are thought to do, and now this recoil has been observed. What’s more, the ejected black hole’s velocity has been measured by analysing the broad spectroscopic emission lines of the hot gas surrounding the black hole (its accretion disk). The ejected black hole is travelling at a velocity of 2650 km/s (1647 mi/s). The accretion disk will continue to feed the recoiled black hole for many millions of years on its journey through space alone.

Supporting the evidence that this is indeed a recoiling supermassive black hole, Komossa analysed the parent galaxy and found hot gas emitting X-rays from the location where the black hole collision took place.

Now Komossa and her team hope to answer the questions this discovery has created: Did galaxies and black holes form and evolve jointly in the early Universe? Or was there a population of galaxies which had been deprived of their central black holes? And if so, how was the evolution of these galaxies different from that of galaxies that retained their black holes?

It is hoped that the combined efforts of observatories on Earth and in space may be used to find more of these “superkicks” and begin to answer these questions. The discovery of gravitational waves will also help, as this collision event is predicted to wash the Universe in powerful gravitational waves.

Source: MPE News

Discovery of Planet Mercury

Ancient people have known about the planets for millennia. It was only in the last few hundred years that new planets have been discovered that required a telescope to see. The earliest people thought of the planets as divine beings, moving across the heavens in unpredictable ways. If you’re wondering about the discovery of Mercury, though, it’s been known since prehistoric times, so there’s no way to really know who made the original discovery of planet mercury.

The five original naked-eye planets were Mercury, Venus, Mars, Jupiter and Saturn, and they had a significant impact on mythology, cosmology, and ancient astronomy. Any caveman could have made the Mercury discovery.

Mercury itself has been mentioned as early as the 2nd millennium BC by the Sumerians, and recorded by the Babylonians – they called the planet Nabu. The ancient Greeks associated Mercury with the god Hermes, who was thought to carry the Sun across the sky in his chariot. Later the Greeks called the planet Apollo when it was visible in the morning sky, and then Hermes in the evening sky. The Romans named the planet after the Roman messenger god Mercury, who was the same mythological figure as the Greek god Hermes.

The first telescopic observations were made by Galileo in the 17th century with his crude telescope; unfortunately, his crude instrument wasn’t powerful enough to see that the planet had phases, like Venus.

Mercury can occasionally be seen to pass directly in front of the Sun, as seen by Earth. This is called a transit. The last transit of Mercury happened in 2004, and was broadcasted worldwide across the Internet. But the first Mercury transit was seen in 1737 by John Bevis at the Royal Greenwich Observatory.

Until the 1960s, Mercury was thought to be tidally locked to the Sun, always facing one side towards our star. There were skeptics, who noted that if Mercury always faced one side towards the Sun, it should have a hot and a cold side, but research data didn’t back that up. Astronomers thought that maybe an atmosphere around Mercury kept the temperatures more even.

In 1962, Soviet scientists bounced the first radar signals off Mercury’s surface, and then American astronomers calculated that Mercury does rotate. It actually takes 59 days to turn once, and not the 88 days it takes to complete an orbit.

The first spacecraft to see Mercury up close was Mariner 10 back in 1974. Unfortunately, it was only able to see one hemisphere of the planet in total over the course of 3 flybys. Many of the missing pieces were filled in by NASA’s MESSENGER spacecraft, which completed its first flyby in January, 2008.

Descubrimiento del planeta Mercurio

References:
NASA Cosmic Distance Scales
NASA Solar System Exploration: Mariner 10

Pictures of Mercury

We can’t just talk about Mercury. Sometimes you’ve just got to see it. Before NASA’s MESSENGER spacecraft, there weren’t a lot of Mercury pictures to choose from. But now the floodgates are open, MESSENGER is sending back more pics of Mercury with each flyby. So here are some of the best photos of Mercury taken so far. I also recommend you to read these amazing books for more information about the planet Mercury.

This first image of Mercury was actually taken by NASA’s Mariner 10 spacecraft, while the others were seen by MESSENGER. As you can see, the new images are so much better than the older ones.



This is one of the first close-up images of Mercury captured by NASA’s MESSENGER spacecraft just before its January 14th, 2008 flyby. It’s a full color image of Mercury, captured by the spacecraft’s Wide Angle Camera (WAC) filters in the infrared, far red, and violet wavelengths (red, green, and blue filters for this image.)



This image of Mercury was captured when the spacecraft was much closer to the planet. The prominent feature is crater Matisse, named after the French artist Henri Matisse. This same crater was imaged by Mariner 10, so this gives scientists a chance to see the difference.



Here’s an image of Mercury’s north pole, captured by MESSENGER during its January 14, 2008 flyby. It’s interesting to note that the planet’s southern regions are much more heavily cratered than its northern regions, which are relatively smooth in comparison. If you read the interesting facts about Mercury, you would know that there could be craters at the planet’s north pole that harbor deposits of ice.



This is a side of Mercury that had never been seen by spacecraft until NASA’s MESSENGER arrived to photograph it on January 14, 2008. Until now, astronomers had only made ground observations of this side of the planet. These images will help astronomers tune their methods and let them compare their ground observations to the close up images captured by spacecraft.

Here are some facts about Mercury.

I’m using Twitter?

I signed up for Twitter a couple of years ago, but I never got around to actually using it. Some part of my brain thinks it would be a great way to do… something. But I have no idea what that would be. I’ll need you to teach me, and help me understand what you’d like to see from my Twitter feed.

Obviously, you don’t want to hear about the minutia of my life, but I think there’s value in great big collaborative conversations. Part of me finds it very exciting, and part of me thinks it’s a time sucking black hole. What am I missing?

Here’s my Twitter feed.

Global Warming is Accelerating Faster than can be Naturally Repaired

It appears the Earth’s climate has the ability to naturally regulate atmospheric carbon dioxide levels. Historic records extracted from ice cores show quantities of CO2 have varied widely in the last hundreds of thousands of years. This evidence appears to support the global warming critics view that current observations of the human-induced greenhouse effect is actually naturally occurring and the effects of carbon on the climate is over-hyped. However, a new study shows that although carbon dioxide levels may have been larger in the past, the Earth’s natural processes had time to react and counteract global warming. The current trend of industrial emissions has been far more accelerated than any historic natural process, natural climate “feedback loops” cannot catch up to remove CO2 from the atmosphere.

More bad news about the outlook for our climate I’m afraid. It would appear that the carbon dioxide emissions we have been generating since the Industrial Revolution have increased too rapidly for the Earth’s natural defences to catch up. This new finding comes from the analysis of bubbles of air trapped in ancient ice in Antarctica, dated to 610,000 years ago.

Long before man started burning coal and oil products, the Earth would naturally generate its own carbon emissions. The main polluters were volcanic eruptions, sending millions of tonnes of carbon dioxide into the atmosphere. Surely this had an effect on the state of the climate? Apparently so, but the increased levels of carbon dioxide produced by individual eruptions could be dealt with naturally over thousands of years. The climate wants to be in balance, should one quantity increase or decrease, other mechanisms are naturally triggered to bring the system back into equilibrium.

These mechanisms are known as “feedback loops”. Feedback loops are common in nature, should one quantity change, production of other quantities may speed up. In the case of the carbon emission from volcanic activity, levels of the stuff appear to have been controlled by a natural “negative feedback” loop (akin to a carbon thermostat, when carbon dioxide levels were too high, another process was triggered to remove the carbon dioxide from the atmosphere). However, the sustained atmospheric input of industrial burning of carbon dioxide by human activity has dwarfed historic volcanic carbon output, overwhelming any natural negative feedback mechanism.

This new study is published in the journal Nature Geoscience and carried out co-author Richard Zeebe. In an interview at the University of Hawaii, Zeebe comments on the climate’s ability to remove carbon dioxide from the atmosphere: “These feedbacks operate so slowly that they will not help us in terms of climate change […] that we’re going to see in the next several hundred years. Right now we have put the system entirely out of equilibrium.”

Zeebe and his team noticed that the levels of carbon dioxide and atmospheric temperature correlated, rising and falling together. “When the carbon dioxide was low, the temperature was low, and we had an ice age,” he said. His study states that in the last 600,000 years the carbon dioxide levels have fluctuated only by 22 parts per million. Since the 18th century, human activity has injected 100 parts per million. Humans have increased the quantity of carbon dioxide 14,000 times more than any natural process is capable of doing. This increase has negated any chance for the climate to naturally bring carbon dioxide levels back down to pre-industrial levels in the short term. If we were to stop all emissions tomorrow, it would take the planet hundreds of thousands of years to recover naturally.

Sadly, we’re not even close to slowing carbon emissions. Only last week, the US reported that carbon dioxide levels were up 2.4 parts per million during 2007 alone. The future is bleak for the planet balancing back into its prehistoric atmospheric carbon equilibrium…

Source: Reuters

Hubble Surprise: Heavyweight Baby Galaxies

Astronomers looking at galaxies in the universe’s distant past were surprised to find some compact, very young galaxies that have masses similar to a mature, grown-up galaxy. Using the Hubble Space Telescope, astronomers discovered nine small galaxies, each weighing in at 200 billion times the mass of the Sun. The galaxies, each only 5,000 light-years across, are a fraction of the size of today’s adult galaxies but contain approximately the same number of stars. Each galaxy could fit inside the central hub of our Milky Way Galaxy.

Using the Hubble in conjunction with Keck Observatory in Hawaii, astronomers were able to study the galaxies as they existed 11 billion years ago, when the Universe was less than 3 billion years old.

“Seeing the compact sizes of these galaxies is a puzzle”, said Pieter G. van Dokkum of Yale University in New Haven, Connecticut, USA, who led the study. “No massive galaxy at this distance has ever been observed to be so compact. These galaxies would have to change a lot over 11 billion years, growing five times bigger. They could get larger by colliding with other galaxies, but such collisions may not be the complete answer. It is not yet clear how they would build themselves up to become the large galaxies we see today.”

To determine the sizes of the galaxies, the team used the Near Infrared Camera and Multi-Object Spectrometer on Hubble. For the Keck observations, a powerful laser was used to correct for image blurring caused by the Earth’s atmosphere. Only Hubble, Keck and ESO’s Very Large Telescope are really able to measure the sizes of these galaxies as they are very small and far away.

The ultra-dense galaxies might comprise half of all galaxies of that mass 11 billion years ago, van Dokkum said, forming the building blocks of today’s largest galaxies.

How did these small, crowded galaxies form? One way, suggested van Dokkum, involves the interaction of dark matter and hydrogen gas in the nascent Universe. Dark matter is an invisible form of matter that accounts for most of the Universe’s mass. Shortly after the Big Bang, the Universe contained an uneven landscape of dark matter. Hydrogen gas became trapped in pockets of the invisible material and began spinning rapidly in dark matter’s gravitational whirlpool, forming stars at a furious rate.

Based on the galaxies’ mass, which is derived from their color, the astronomers estimated that the stars are spinning around their galactic disks at roughly 400 to 500 kilometers per second. Stars in today’s galaxies, by contrast, are traveling at about half that speed because they are larger and rotate more slowly than the compact galaxies.

The astronomers say that these galaxies are ideal targets for the Wide Field Camera 3, which is scheduled to be installed aboard Hubble during upcoming Servicing Mission 4 in the fall of 2008.

Original News Source: European Hubble Space Telescope Homepage