Into the Brown Dwarf Desert

At first glance, the object called COROT-exo-3b doesn't seem all that interesting. True, planets that orbit remarkably close to their stars were a surprise when first detected, but we've since found enough of them to know that a gas giant in a four-day orbit, which is about how long this object takes to circle its star, is not a great rarity. We've also learned that radial velocity methods are going to detect large, close objects more quickly than planets that orbit farther from their primary. Why is COROT-exo-3b making news? Then you look a little more closely at the new find. For one thing, the COROT mission depends not upon radial velocity measurements but planetary transits. More significantly, COROT-exo-3b is roughly the size of Jupiter but is fully twenty times as massive. Orbiting an F-class dwarf with metallicity values much like the Sun, the object opens up a new perspective, for we've found planets twelve times as massive as Jupiter and stars seventy times as massive, but...

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A Sparsely Populated Kuiper Belt?

The transit method -- observing a distant planet as it moves in front of its star as seen from Earth -- is a prime tool for exoplanet detection. But transits are hardly limited to planets around their primaries. The Taiwanese-American Occultation Survey (TAOS) is demonstration of that, an attempt to find tiny Kuiper Belt objects (KBOs) in the range between 0.5 and 28 kilometers. As you would imagine, at a distance like this such objects cannot be seen directly, but an occultation -- the dimming of a star when one of the KBOs passes in front of it -- should be apparent. The image below shows the method applied to a cometary nucleus. Image: Looking for dimmed starlight -- the basic method at work in the TAOS survey. The experiment follows 3000 stars five times per second in its search. Credit: TAOS. TAOS works with small, wide-field robotic telescopes on peaks near the Yu-Shan (Jade Mountain) National Park in Taiwan. The current results represent 200 hours of collected data using these...

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A Copernican Space Imperative

I'm a great admirer of Princeton astrophysicist Richard Gott, who periodically breaks into the popular press because of his quirky predictions about the human future. This is not to say that I necessarily agree with his applications of the Copernican principle, many of which have proven accurate, but rather that long-term predictions ignite both my native skepticism and my fascination with what may be coming down the road. And Dr. Gott says intriguing things indeed, such as this response to the Fermi question: 'Where are the extraterrestrials?...a significant fraction must be sitting on their home planets." As you would imagine, controversy follows such thoughts, and the follow-on that we are probably a rather typical civilization with only a tiny window for getting into space that should be exploited as soon as possible. Most species go extinct -- will we be any different in the face of pandemic, nuclear war or incoming asteroid? The latest Carnival of Space is now up at Alice's...

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Changing How We See

Again and again I'm amazed by our growing ability to tease information out of apparent noise. Consider the problem of viewing celestial objects from Earth's surface. The image below demonstrates the latest way to remove atmospheric blur that would otherwise bedevil a ground-based telescope. We're looking at Jupiter through a prototype instrument called the Multi-Conjugate Adaptive Optics Demonstrator (MAD). This is a form of adaptive optics that uses two guide stars (or in this case, two of Jupiter's moons) instead of one as references, allowing a wider field of view. Adaptive optics involves real-time corrections made at high speed, feeding a computer-controlled deformable mirror that interprets the atmospheric distortion by examining light from the chosen guide stars. Normally, the method works with a single guide star, but that allows for atmospheric corrections only in a tiny region of sky. The new MAD methods significantly overcome this limitation. The false-color infrared...

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Laser Beamed Interstellar Mission: A New Take

For all their attraction as a way to leave weighty propellant behind, solar sails have a fundamental limitation. Their power source is the Sun. As you move away from the Sun, the amount of available light drops according to the inverse square law -- a spacecraft that doubles its distance from the Sun encounters only a fourth of the sunlight previously available. Quadruple the distance and the sunlight drops to a sixteenth of what it was, making sail operations problematic in the outer Solar System. And what of the stars? Solar sail specialist Greg Matloff has been juggling the numbers on interstellar travel via solar sail for decades now, and even with the best case scenario involving an extremely close solar pass, a thousand years to Centauri is about as good as it gets. And that's quite a stretch in itself. Epsilon Eridani would actually make an easier mission as it's much closer to the ecliptic, so you get 30 kilometers per second (Earth's orbital velocity around the Sun) from...

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Galaxy Survey: An Intriguing M81

Hubble's ACS Nearby Galaxy Survey Treasury (ANGST) has everything going for it but the right acronym. One thing the spectacular images returned from this work definitely do not lead to is a deep, philosophical fear or, as 'angst' is defined by the American Heritage Dictionary, "A feeling of anxiety or apprehension often accompanied by depression." Quite the contrary, the results of ANGST are all but euphoric in their celebration of stars in the galaxies we see around us, fully sixty nine galaxies in the so-called 'Local Volume.' The euphoria comes from Hubble's sharp vision. The Local Volume encompasses galaxies beyond the Local Group, with distances in the survey ranging from 6.5 million light years to 13 million light years from Earth. That's actually close enough that the right tools for seeing -- Hubble's Advanced Camera for Surveys and Wide Field Planetary Camera 2 -- can pull individual stars out of what had been an indistinct galactic background. Out of that we stand to learn...

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Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

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