This 219th meeting of the American Astronomical Society meeting is under way this week in Austin, TX. There will be lots of scientific talks, posters, and in-the-hallway discussions between the 2,700 astronomers who have come to Texas for the meeting. (That's quite a bit when you consider there are probably only several thousand professional astronomers in the whole US!)
Of course, there are lots of Chandra results being shared. Tomorrow, there will be a press conference to announce some exciting new findings involving Chandra and some of the largest objects in the Universe. We'll have the news posted on our website at 10am Central so check back for the latest in the X-ray Universe.
-Megan Watzke, CXC
Dr. Giuseppina (Pepi) Fabbiano is a senior astrophysicist at the Smithsonian Astrophysical Observatory where she studies, among other things, galaxies, black holes and the rest of the high-energy Universe using Chandra and other telescopes.
It would be fair to say that I stumbled into astronomy. I grew up in a family of teachers, professors and professionals, both men and women, and there never was any doubt that I had to go to university and then get a good job. I was a precocious learner and always ‘first of the class.’ I won the math prize in high school and was one of a busload of high school students from the whole of Italy rewarded with a prize visit to France.
Today, a new leader reports to NASA HQ to take over what is known as the Science Mission Directorate, or SMD. SMD is the branch of the agency that is responsible for all things science at NASA - from heliophysics to Earth science to planetary science and astrophysics. Chandra, as well as the other "Great Observatories" missions of Hubble and Spitzer, and many, many missions belong to the astrophysics realm of SMD.
With the holiday season in full swing, a new image from an assembly of telescopes has revealed an unusual cosmic ornament. Data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton have been combined to discover a young pulsar in the remains of a supernova located in the Small Magellanic Cloud, or SMC. This would be the first definite time a pulsar, a spinning, ultra-dense star, has been found in a supernova remnant in the SMC, a small satellite galaxy to the Milky Way.
This year, the winter solstice takes place on Thursday, December 22 at 12:30 a.m. EST. Many people know that the winter solstice marks the day when winter officially stars in the Northern Hemisphere, and when days will start to become incrementally longer. But what exactly is going on?
It all has to do with the tilt of the Earth's axis. In other words, the Earth does not rotate on its axis straight up and down in relation to its path around the Sun. Rather, it is always angled at 23.5 degrees. So as the Earth travels around the Sun during the course of the year, one pole is tilted more toward the Sun that the other with the exception of two days: the vernal (spring) and autumnal (fall) equinoxes.
One of the projects that we're very excited around here is something called "Stop for Science!" (aka, STOP). This is a program aimed at engaging kids outside of classroom time in thinking about science. STOP is meant to be fun, but also informative. The centerpiece of the program is a series of five posters covering different areas. The topics range from "how tall is tall" to "when stars go boom." Each poster has accompanying material including background information, questions for different ages of kids, and teacher resource guides.
Like wine in a glass, vast clouds of hot gas are sloshing back and forth in Abell 2052, a galaxy cluster located about 480 million light years from Earth. X-ray data (blue) from NASA's Chandra X-ray Observatory shows the hot gas in this dynamic system, and optical data (gold) from the Very Large Telescope shows the galaxies. The hot, X-ray bright gas has an average temperature of about 30 million degrees.
While most of us in the US were still digesting from the Thanksgiving holiday this past weekend, many folks at NASA were incredibly busy. That's because on Saturday, November 26th, NASA launched the Mars Science Laboratory (MSL) into space aboard an Atlas V rocket.
Q: Can black holes move through space?
A: Black holes can indeed move through space. The really massive black holes at the centers of galaxies will stay there unless something catastrophic happens, like a direct collision between two galaxies.
On the left, an optical image from the Digitized Sky Survey shows Cygnus X-1, outlined in a red box. Cygnus X-1 is located near large active regions of star formation in the Milky Way, as seen in this image that spans some 700 light years across. An artist's illustration on the right depicts what astronomers think is happening within the Cygnus X-1 system. Cygnus X-1 is a so-called stellar-mass black hole, a class of black holes that comes from the collapse of a massive star. The black hole pulls material from a massive, blue companion star toward it. This material forms a disk (shown in red and orange) that rotates around the black hole before falling into it or being redirected away from the black hole in the form of powerful jets.
Please note this is a moderated blog. No pornography, spam, profanity or discriminatory remarks are allowed. No personal attacks are allowed. Users should stay on topic to keep it relevant for the readers.
Read the privacy statement