A new Star in our Universe?

On the heels of 1651-32 V1280 Scorpii (a.k.a. Nova Scorpii 2007), the "new star" discovered earlier this month in the constellation Scorpius, observers in Japan think they may have found another. The reputed nova is reportedly shining in the range of magnitude 9.2 or 9.3, which makes it visible with binoculars.On February 21, the American Association of Variable Star Observers (AAVSO) Special Notice #34 reported that Yuji Nakamura — one of the observers who found Nova Scorpii 2007 — and Hideo Nishimura independently discovered the possible second nova.

A nova, or "new star," recently discovered this month in Scorpius has brightened so much in recent weeks that it is now visible to the naked eye. Officially christened Nova Scorpii 2007, the nova is a star whose brightness has suddenly and dramatically increased.

Nova Scorpii 2007 brightened steadily from February 8 to 16, when it peaked at approximately magnitude 4. The magnitudes in this graph are daily averages based on data observers reported to the American Association of Variable Star Observers. Astronomy: Roen Kelly [larger image]
The nova was discovered independently by two Japanese observers, Yugi Nakamura and Yukio Sakurai. On February 7, the American Association of Variable Star Observers (AAVSO) reported the nova's approximate brightness as magnitude 8.3. It peaked in brightness February 16 at about magnitude 4, according to the average brightness calculated from raw data posted by the AAVSO. On February 20, the AAVSO posted fresh observations showing that Nova Scorpii 2007 had dimmed to approximately magnitude 4.7.

To find the new star, locate Scorpius in the morning sky and use the finder chart here to locate Antares, Scorpius' brightest star. Then look down and a bit to the left to locate Nova Scorpii 2007. The nova is about the same brightness as the dim star in Orion's head. It will be easily visible with binoculars.

Europa's potential for life

Jupiter with Europa & Callisto

There are four large, moons of Jupiter that in their character and behavior are more like planets than Earth's moon: Io, Europa, Ganymede and Callisto. The last three are icy.
Io's volcanic hyperactivity is well known, but there are mysteries about the temperature of its magmas and its spectacular mountains and what they might reveal about the satellite's interior processes. As for the exterior moon Callisto, how did it acquire an ocean yet not be deeply differentiated? Ganymede's liquid iron core is still generating a magnetic field. This was not predicted beforehand, and thus has much to teach planetary scientists on how magnetic fields are generated in the solar system.

Then, there is Europa.
"Of the four Galilean moons, Europa is the one that has the best chance to reveal the most about the origin of life, which is the biggest unanswered scientific question we have, bar none," he said. "With its massive body of liquid water, multiple energy sources proposed and different ways to provide carbon and other biogenic elements, the central question must be Europa's potential for life. What greater question can you ask of a planet?"
McKinnon reviewed each of the moons and their unanswered questions in his invited talk, "O Sister, Where Art Thou? The Galilean Satellites After Galileo," presented at the Fall 2006 meeting of the American Geophysical Union held Dec. 10-15, 2006, in San Francisco. All but Ganymede, a young male, are named after female Greek mythological characters. Thus, McKinnon refers to Ganymede as an honorary sister.
"Europa has been recently geologically active, but because Galileo's main antenna did not unfurl, we did not take enough images to catch any active geysering, such as seen on Saturn's itsy bitsy icy moon, Enceladus," McKinnon said. "Europa's surface appears very young and there are lots of interesting ice tectonics, and surface eruptions with weird colors and spectral signatures whose compositional implications everyone just loves to argue about."
'Capped' ocean
All the accumulated evidence points to an ocean under a global shell of ice, an ocean lying no more than 10 to 20 kilometers below Europa's airless surface, McKinnon said.
"That sounds really deep to a person with a pick ax, or even a drilling rig, but in geologic terms it's really pretty close," he said. "It's basically a capped ocean. "
The existence of the ocean is related to the great amount of heat coming up from Europa's interior.
"If you look at the surface and how deformed it is, you can tell the ice shell is relatively thin and really has been active in recent geological time, indeed is probably active today," McKinnon said.
Europa has a few, but not many, impact craters, also indicating its relative youth.
Europa's ocean begs to be studied, McKinnon said, as do the strikingly colored surface materials that Galileo images captured.
"To go into orbit around Europa with high-resolution cameras, spectral imagers and sophisticated, ice-penetrating radars of the sort mapping Mars right now, would allow us to really characterize that ocean and give us clues about the biogenic potential of the surface materials, "McKinnon said. "We'd see to the bottom of the ice shell, I predict. It would be a fantastic proof of concept."
A mission to Europa is feasible, McKinnon said. It would take about 10 years if started today (six of those years being spent in reaching the satellite). And it would be expensive, "about two billion dollars, give or take," he added.
"It would also have to compete for funds with NASA's plans to establish a Moon base," he said. "The Europeans are interested as well, so maybe we could cooperate and share the cost."
NASA has committees exploring a number of options, McKinnon said, and they include returning to Europa or Titan after the conclusion of the Cassini mission or perhaps returning to the little active moon around Saturn, Enceladus.
"It's a tiny moon, but it has an active plume that, because of that moon's very low gravity, extends well out into space, so you can just fly right through it," McKinnon said. "That's a nifty way to go sampling."
Of course, Europa is a much bigger target to explore.
"It has 40 times the surface area of Enceladus — there's a lot more there there," he concluded.

Cosmology is the study of the overall structure of the universe. Just what is the Universe? It is everything that exists. However, from Earth we cannot observe everything in the Universe. Some things are dark (brown dwarf stars, planets, and Dark Matter) and we cannot see them. Additionally, there are parts of the universe whose light has not yet reached us in this part of the Universe. And because light travels at a set speed we actually look back in time when we look into the cosmos.
Astronomers observe some interesting structure in the Current Universe. That structure can tell us much about the History of the Universe. It can also tell us what we can expect for the Future of the Universe and beyond...

A computer simulation depicting a large chunk of our universe