HLX-1 (Hyper-Luminous X-ray source 1) is thought to be a black hole, one that's a welcome discovery for astronomers trying to puzzle out the mysteries of black hole formation. Located roughly 290 million light years from Earth and situated toward the edge of a galaxy called ESO 243-49, this black hole looks to be some 20,000 times the mass of the Sun, which makes it mid-sized when compared with the supermassive black holes at the center of many galaxies. The latter can have masses up to billions of times more than the Sun -- the black hole at the center of our own galaxy is thought to comprise about four million solar masses. Just how a supermassive black hole forms remains a subject for speculation, but study of HLX-1 is giving us clues that point in the direction of a series of mergers of small and mid-sized black holes. For it turns out that HLX-1, discovered by Sean Farrell (Sydney Institute for Astronomy in Australia and University of Leicester, UK) and team at X-ray...

Luminous Blue Variables are large, bright stars that give rise to periodic eruptions, like the so-called “Great Eruption” of Eta Carinae that was first noted in 1837 and continued to be observed for an additional 21 years. Things must have been lively around the companion star thought to orbit in the nebula around Eta Carinae, for the LBV blew off about 20 solar masses in this era, mimicking a supernova as it became the second brightest star in the sky. We’ve witnessed similar ‘supernova impostor’ events in other galaxies, but at 7500 light years, the Eta Carinae system is relatively nearby, allowing close study by Hubble and other telescopes. What brings Eta Carinae’s 1837 event back into the news is the use of so-called ‘light echoes’ to study what happened at a time when astronomy was in a much earlier state. Armin Rest (Space Telescope Science Institute) notes how useful the work is turning out to be: "When the eruption was seen on Earth 170 years ago, there were no cameras...

The Planck mission continues to peel the layers off the onion as it probes the early universe. Planck is all about the Cosmic Microwave Background (CMB), that radiation left over from the era of recombination around 380,000 years after the Big Bang. As electrons and protons began to form neutral atoms, light was freed to stream through the universe, an afterglow of the Big Bang that missions like the Wilkinson Microwave Anisotropy Probe have studied in detail, and which Planck will now observe at still better sensitivity, angular resolution and frequency range. But the initial job for researchers is to remove sources of foreground emission to reveal the CMB itself, and that process is turning up interesting findings in its own right. The latest announcement from the European Space Agency involves a haze of microwaves that is not yet understood. Coming from the region around galactic center, the haze appears to be synchrotron emission, produced as electrons accelerated in supernovae...

Given yesterday's post on wandering planets, otherwise known as 'rogue' planets or 'nomads,' today's topic falls easily into place. For even as we ponder the possibility of 105 rogue planets at Pluto's mass or above for every main sequence star in the galaxy, we confront the fact that we still have much to learn about objects much closer to home in our own Kuiper Belt. We have yet, for example, to have a flyby, although it's possible the New Horizons spacecraft will line up on a useful target after its encounter with Pluto/Charon (and yes, it's conceivable that Triton is a captured KBO, and thus we have had a Voyager flyby). The discovery of objects like Sedna, Makemake and Eris makes it clear how much we may yet uncover. We can think of the broader category of Trans-Neptunian Objects (TNOs) in terms of potential mission targets, but we should also ponder the fact that their strong dynamical connection with the planets can help us gain insight into the mechanics of Solar System and...

Not long ago we looked at comet C/2011 N3 (SOHO), discovered last July just two days before it plunged into the Sun, evaporating some 100,000 kilometers above the solar surface. It was startling to learn that the SOHO observatory is tracking numerous ‘Sun-grazers,’ comets whose fatal encounters with our star are occurring roughly once every three days. Now comes news that Sagittarius A*, the supermassive black hole at the center of the Milky Way, is producing X-ray flares about once a day, thought by some to be the result of similar debris in the process of destruction. The flares last just a few hours, according to researchers working with data from the Chandra X-Ray Observatory, and can reach brightness levels up to 100 times what is normally observed in the black hole region. Kastytis Zubovas (University of Leicester) thinks we’re seeing asteroids and comets passing within 160 million kilometers of the black hole (roughly 1 AU), at which point they would likely be broken apart by...

Gravitational lensing always gets my attention not only because of its growing use in astronomy but because of its potential for deep space missions like FOCAL, Claudio Maccone's concept for a deep space probe that would be sent beyond the Sun's 550 AU gravitational lensing distance to make observations of astronomical targets. FOCAL is an interstellar precursor mission that could give us detailed information about any system to which we might send a future probe. And, as Maccone has shown, lensing could also be used to create the kind of robust communications relay that would function with little data loss over huge distances. But we don't have to wait for FOCAL to exploit the potential of lensing for studying distant exoplanets. As Centauri Dreams readers know, gravitational microlensing has developed into a potent tool. A foreground star distorts the light from a background object when the alignment is right, and that magnification is likewise affected by planets orbiting the...