Where:

Frosty Drew Observatory

When:

Friday February 12, 2016 at 6:00 p.m.

Cost:

$1 Suggested Donation per Person

Tonight is Stargazing Night at Frosty Drew Observatory and forecasts are looking rather unfavorable. We can expect increasing clouds this afternoon, becoming fully cloudy by sunset with snow showers moving in overnight. This is rather unfortunate since tonight's 22% waxing crescent Moon would have offered up stunning views of the lunar surface and Earth-shine (when sunlight reflects off the Earth and illuminates the shadow side of the Moon). Extremely cold temps are also making their way into the region, making for a dangerous situation for those dressed inadequately.

We plan to open the Observatory and Sky Theatre at 7:00 p.m. tonight. In the Observatory, tours of our telescope and operations will be available. These are the nights where we keep the lights on and all the awesome things that make the Frosty Drew Stargazing Nights happen are in plain view. In the Sky Theatre we will feature a showcase of celestial objects we photograph at Frosty Drew with a commentary and open discussion on general astronomy. We will stay on site and open until 9:00 p.m.

Overall, tonight's conditions will likely keep celestial goodness just beyond our ability to sneak a peek. Though the Sky Theatre will be warm and buzzing with astronomy, making tonight a perfect chance to get some answers to those obscure astronomy questions you've been pondering, catch up on the gravitational wave discovery, or just to grab a quick astro-fix. If you have a free night, stop in and have a astro-geek-out with us.

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Weekly Happenings
Scott MacNeill

Yesterday morning, February 11, 2016, the announcement that took the astrophysics world by storm was set loose. Gravitational waves have been directly detected. This discovery, again, proves how spot on Einstein's view of the cosmos was when he predicted the existence of gravitational waves in 1916 as part of his general theory of relativity. The direct detection of gravitational waves offers us a new method of observing and studying the Universe.

Gravitational waves, as predicted by Einstein, are ripples in the fabric of space, called space-time, that travel at the speed of light. These ripples are a result of catastrophic events in the Universe, events like supernovae, fast orbiting neutron stars, the big bang, and in this case a binary black hole merger (two black holes orbiting each other and eventually merging into one larger black hole). Einstein's mathematical predictions show that massive objects that are accelerating would disrupt space-time around them causing waves of distorted space to radiate from these massive objects. These waves would compress and expand space-time as the wave passes, in a similar fashion to ripples moving across the surface of water.

Detecting gravitational waves is difficult. Space-time distortions created by gravitational waves would measure 10,000 times smaller than the width of a proton. To capture these tiny distortions, the LIGO detectors were devised and built. Each detector, one located in Livingston, Louisiana and another located Hanford, Washington, are comprised of two 2.5 mile long perpendicular arms that make up a visible “L” shape. Inside each arm are a series of mirrors that reflect a laser beam, from a single source, back and forth along the 2.5 mile distances. After traveling the length of the arm about 400 times, due to reflection, the laser beams merge and are sent to a photodetector. The exact distance each laser beam travels should match precisely. Unless a gravitational wave passes over, which would cause a tiny difference in the distance of both beams.

Now there are many local anomalies and events that could produce a similar effect of a gravitational wave. That is why multiple identical detectors are required. When a gravitational wave propagates over Earth, all detectors should detect the same differences in distance the laser beam travels along its designated arm of each detector. Essentially, any event that is not detected by both detectors and that doesn't match will be considered noise and removed from the recorded data sets, allowing for detection of real gravitational waves.

On September 14, 2015, both LIGO observatories measured the same distortion with only a 7 millisecond difference in detection time. Since gravitational waves move at the speed of light and the Livingston, LA observatory recorded it first, we are able to predict that the source of the gravitational wave came from the Southern Hemisphere skies. Measuring the amplitude of the wave enabled us to calculate 1.3 billion light years as the distance to the event that caused the gravitational wave, which was the merger of two black holes in a binary black hole system, where both black holes orbited each other and eventually merged into one large black hole.

This discovery is monumental to better understanding the cosmos. Detecting gravitational waves enables us to observe the Universe in a completely new method never before possible. Traditionally, all observations are made using electromagnetic radiation (radio, microwave, infrared, visible, ultraviolet, x-ray, and gamma ray), which interacts with matter. Gravitational waves move through the Universe unaffected by matter, offering us an unaltered view into the events that caused them. Gravitational waves also contain information that electromagnetic radiation does not. Consider a black hole, which emits almost no electromagnetic radiation. The gravitational waves emit by the black hole will be visible to detectors like LIGO, allowing us to further detect and study these obscure groups of objects. This discovery just opened the door to a much larger view of the amazing Universe we are part of, where awesome things are just around the cosmic corner!

-Scott