Rosetta’s Final Mission

Tomorrow, one way or another, the ESA’s Rosetta mission is coming to an end.  In a final maneuver, the craft will attempt to land on the surface of the comet, following in the footsteps of the Philae lander, though hopefully with more success. The video shows the final orbit plan, and really highlights how amazing mission scientists are to be able to plan a landing site when the comet is rotating so quickly, relative to the craft’s motion. You can follow the link to watch the live broadcast of the event here.  The mission will end around 7:20am EST tomorrow,...

Hunt for the Small and Slow

With the recent discovery of gravitational waves, we now have a target for probing the very early universe, close to the big bang.  This is because gravitational waves can travel across the universe unimpeded, meaning those created after the big bang are still bouncing around today.  It’s like the big bang was the ringing of a giant bell, and the ringing can still be heard.  But all of our Easter eggs are not in one basket.  There is another way to probe the very early universe, one we haven’t found yet, because it involves particles that are very tiny and...

Edge-On: Good for Planets, Bad for Galaxies

Every time we see amazing photos of galaxies or planetary disks, we can see most of the detail since we see them face on.  But since the orientation of spiral galaxies in the universe is random, there are a plethora of galaxies ignored by image processors since we just can’t see much of the detail.  We can still learn from edge-on spiral galaxies, just not as much as we can from those that are face on. We can see some fascinating dust lanes in the image above, and a ton of detail considering the view, but we don’t know what...

Precision and the Prime Meridian

The Prime Meridian is the imaginary line of zero longitude, the geographic starting point for any East-West degree measurement of any place on the Earth.  It was selected by an international delegation that convened in 1884 in Washington, DC.  It’s a North-South imaginary line that run right through the Airy transit circle at the Royal Observatory in Greenwich, England.  This is also where we get the measurement of Greenwich Mean Time (GMT). As our ability to measure position and time improves with the Global Positioning System (GPS), the precise position of the prime meridian has actually changed, moving 102 meters East...