Category Archives: astronomy

Clusters Moving along in a Dark Flow

Scientists Detect Subtle Cosmic Motion

Hot gas in moving galaxy clusters (white spots) shifts the temperature of cosmic microwaves. Hundreds of distant galaxies seem to be moving toward on patch of sky (colored purple). NASA/WMAP/IA Kashlinsky, et al.
Hot gas in moving galaxy clusters (white spots) shifts the temperature of cosmic microwaves. Hundreds of distant galaxies seem to be moving toward on patch of sky (colored purple). NASA/WMAP/IA Kashlinsky, et al.

Oh hey, now this is neat. Complex, but neat. A team led by astronomer Alexander Kashlinsky at NASA’s Goddard Space Flight Center, is looking out at distant clusters of galaxies have been tracking the motions of those clusters as they move through space. And, they’ve found something unexpected, something they are calling “dark flow.”  Essentially, the motions of those clusters have a little “outward tug” that seems to imply a gravitational attraction by something (matter) that lies beyond the cosmic horizon. This tug is independent of the clusters’ own motions and it can’t be accounted for by the expansion of space.

How did astronomers find this dark flow?  They used the Wilkinson Microwave Anisotropy Probe (WMAP) to measure the photons of microwave light as they pass by and are scattered by hot x-ray-emitting gases in the clusters. Essentially, the astronomers dug into the spectra of the scattered light to look for a very tiny shift in the microwave background’s temperature in the direction of the clusters. They looked at a large number of clusters using the technique and found this motion that seems to affect clusters up to 6 billion light-years away. When they measured the motion, they clocked it at nearly 3.2 million kilometers per hour and its direction of flow points directly at a 20-degree-wide patch of sky between the constellations Centaurus and Vela.

What does this mean? You can read more about the finding in a Goddard press release. Essentially, however, astronomers are still refining the measurements, but it seems safe to say that it means stuff is moving faster at greater distances than they expected. And, it’s directional, which is challenging to explain unless you invoke some kind of gravitational influence of unseen matter in the attracting region.  What’s there?  Good question.  Stay tuned!

What’s Scrubbing the Plasma Conduits?

Solar Wind Levels Down

The solar heliosphere
The solar heliosphere

The Ulysses spacecraft (the one I wrote about a few months back that’s nearing the end of its mission) has measured the lowest levels of solar wind output in 50 years (since the beginning of the Space Age). What’s going on with the Sun? And, does this have implications for Earth?

The solar wind plasma is a stream of charged particles ejected from the Sun’s upper atmosphere. It flows past and interacts with every planet in our solar system. The solar wind ebbs and flows as solar cycles come and go, and right now there’s minimal activity on the Sun. In fact, it has been in a state of low activity for much longer during this current solar cycle than astronomers expected.

So, how does this affect Earth?  Let’s talk about the protective properties of the solar wind. Its far limit (that is, the edge of the expanding “bubble” blown out around the solar system by the solar wind) pushes against the interstellar medium. That limit is called the “heliopause.”  It acts as sort of an umbrella to protect the rest of the solar system against winds from other stars and wards off a significant portion of cosmic rays (high-energy particles) from outside the galaxy.

Galactic cosmic rays are radiation carriers, and if the heliopause gets smaller and weaker (and since the solar wind is at an all-time low, there could be some diminishment of the protective barrier of the heliopause), more galactic cosmic rays could make their way to the inner solar system–and Earth. How this affects us depends on much gets through. But, it’s not a dire thing. The heliosphere isn’t collapsing. Far from it. But, these measurements of solar wind output from Ulysses are giving us a new look at solar activity. Is it normal for the Sun to be so quiet? To ramp down its solar wind?  Good questions.