Wright Brothers

First Powered Flight

During a recent beach vacation on North Carolina's Outer Banks we visited the Wright Brothers National Memorial in Kitty Hawk. At this spot, on December 17, 1903, the first powered flight took place. A stone marker, dedicated in 1928, now stands at the launch point. A replica of the launching rail leads to the spot where the airplane lifted off as you can see in the picture below.

The following sign explains the role of the launching rail. (Click on the image to more easily read the text.)

Amelia Earhart was present along with Orville at the 1928 dedication.

The first three flights were only short hops before a much longer fourth flight took place as explained by this nearby sign. (Click on the image for a better view.)

The endpoints all four flights are marked with stones. We were too lazy to walk all the way to the fourth stone in the heat.

The present day memorial has recreated the crude 1903 buildings used by the Wright brothers. One is a hanger, and the other served as a workshop and living quarters.

South of the first flight stone marker is a larger monument erected on Kill Devil Hill. The park ranger explained how the present hill is roughly 200 yards or so from where it was located when the Wrights used it for glider experiments. The hill and surrounding ground were all bare sand in 1903, and the huge hill/sand dune migrated to its present position due to the natural action of winds. Vegetation was added to halt further migration, and you can see grass now covering the original sandy field.

On the south side of Kill Devil Hill sculptor Stephen Smith created a magnificent life size reproduction of the moment the first flight took off. It was hard to get pictures without other visitors in the photos. Next is a panorama showing the entire sculpture. (Click on the image for a larger view.)

The next two pictures show members of the Kill Devil Hills Life-Saving Station who helped the Wright Brothers move the plane and then witnessed the first flight. One of them, John Daniels, took the famous historical first flight photo.

The Wright brothers had flipped a coin to decide who would pilot the first flight. They took alternating turns thereafter. Wilbur made an unsuccessful try on December 14th, therefore, it was Orville's turn to try three days later on December 17th. The sculpture shows Wilbur running alongside as the plane lifts off under his brother's control.

Here's the plane with Orville at the controls next to the motor.

It's hard to believe this contraption actually flew!

I loved this sculpture! It was the best part of the Wright Brothers National Monument.    

Few Solar Features

Approaching Solar Minimum

My solar telescope has been idle for eight months. During this time good observing conditions did not coincide with the presence of significant solar features. The Sun's roughly eleven year sunspot cycle is probably within a year of reaching minimum activity, so sunspots are rare these days.

Sunspots and large filaments have been mostly absent from the solar disc for many months. What a change from three years ago! In 2015 there wasn't a single day without sunspots. By 2017 there were 104 spotless days, about 28 percent of the time. So far this year the sun has been spotless 54 percent of the time. Any recent sunspots have usually been small and short-lived.

On May 24th a week of rain and clouds finally ended leaving lower humidity and a clear blue sky over my red dot location in eastern Virginia as you can see in the following satellite image taken that day.

Although few solar features were present, I decided to do some imaging anyway. Gentle puffs of breeze blew from time to time. The temperature ranged from a tolerable 75 to 78 degrees. Observing conditions would have been nearly perfect except for neighborhood noise. String trimmers and lawn mowers roared next door while a screeching rock saw cut patio stones for another neighbor. Occasional dust clouds from stone cutting blew towards my yard.

A bit out of practice with the solar observing routine, I took my time and consulted notes. Eventually, I captured some decent images. The first picture below is a 15-panel mosaic showing modest features on the eastern half of the Sun. Active area 2712 had just rotated into view near the limb. Active area 2710 is to the right of 2712. A number of prominences are visible around the limb. (Click on the image to see better detail.)

Aside from two small active areas seen above, the remaining eastern solar surface is relatively featureless. The next picture is a two-panel mosaic showing a closer view of the two active areas. During the time of image capture area 2712 on the left had emitted a small jet of gas toward the limb.

Area 2710 showed only the characteristic white color of increased energy emission but no sunspot umbra.

The Sun's west side contained only one obvious sunspot umbra contained within active area 2711 seen below.

I used longer exposure times to capture relatively dim prominences along the eastern limb. The brighter disc was, consequently, overexposed. I've blacked out the disc in the next 7-panel mosaic so only limb features are visible. Unfortunately, software used to combine separate images into a mosaic slightly distorted the limb from its true circular shape. The distortion isn't drastic, but it's definitely noticeable in the image below. (Click on the image for better detail and less apparent distortion.)

Longer exposure times did reveal more prominence features than those visible in the first mosaic image above.

As the solar activity cycle grinds through its minimum over the next year or so I'll have to patiently wait for good opportunities to observe. 

Insects in Amber

Frozen in Time

Amber is ancient solidified resin. Long ago, while still viscous and sticky, the resin may have engulfed bits of leaves, pine cones, seeds, or insects. Under the right conditions, over time, the resin hardened. With luck, the hardened resin, along with its cargo of trapped contents, got beautifully preserved as solid amber.

Particularly large amounts of amber are found along the shores of the Baltic Sea in northern Europe. In 2001, while visiting Krakow, Poland, I purchased the small piece of insect bearing amber shown magnified in the first picture below. Although it is only about two centimeters long, it contains three insects! The bugs look somewhat like mosquitoes, but without the blood sucking proboscis. They could be small flies called midges. I'm not an expert, so I don't really know what these bugs are. I have no exact age for this particular piece, but Baltic amber is determined to come from approximately the Eocene Era, roughly 54 to 34 million years ago.

Another source of amber is located in the Dominican Republic. Dominican amber formed from the resin of extinct Hymenaea trees during the time of the Oligocene and Miocene Eras, about 30 to 20 million years ago. During my recent visit to the New Jersey Mineral, Fossil, Gem and Jewelry Show I purchased three bits of insect bearing Dominican amber. The next picture shows what looks like a grasshopper leg beautifully suspended within light colored Dominican amber.

All pictures here were taken with a Samsung Galaxy 8 Plus phone camera handheld to the eyepiece of a low power microscope. It was a challenge to hold the camera steady, arrange suitable lighting, and achieve good focus on the insects themselves. As you can see in the three pictures below, results were not always crisp and clear. The next picture shows another piece of Dominican amber. Details of the unknown bug within are blurred by blemishes in the amber.

Next is a magnified image of the unknown bug. There seems to be a wing sticking out the back.

Finally, three insects are suspended within my third piece of Dominican amber shown in the last picture below.

It's astounding to think these trapped insects were alive 20 to 40 million years ago! They lived in a world inhabited by animals now extinct. Nothing remotely resembling a modern human was alive. Even the arrangement of seas and continents around the globe was different than it is today. Yet, through wonderful natural process that produce amber, I can now hold these preserved examples of ancient life in my hand.

Radioactivity

Invisible Radiation

I purchased a small radioactive specimen at the recent New Jersey Mineral, Gem, Fossil and Jewelry Exhibition. Although the dealer assured me the radiation level was completely safe, I was curious about the actual amount. Eventually, I bought an inexpensive radiation detector to measure the radiation myself.

The detector pictured above has a small Geiger-Muller tube located inside the plastic case along the bottom. It detects beta, gamma, and x-rays. According to the user manual, it is sensitive to gamma rays with energies between 0.1 and 1.25 Mev and beta rays with energies between 0.25 and 3.5 Mev. The given x-ray energy range in the manual was probably printed incorrectly, so I don't know the x-ray values. The detector can register each particle with an audible click, and it sounds an alarm when the count rate exceeds 100 counts per minute.

Upon receiving the detector I immediately measured radiation count levels at various places around my house. I let the detector count for 10 minutes and calculated the average count rate for this amount of time. The count rate is measured in counts per minute, or CPM.

• At the dining room table the average count rate was 20 CPM.
• On the granite kitchen counter the average count rate was 20 CPM.
• At the computer in my "office" the average count rate was 16 CPM.
• On my bed the average count rate was 17 CPM.

All these values are described as "safe, no worry at all" in the detector's user manual. They apparently represent normal background radiation in my house. Any count rate below 50 CPM is classified as safe according to the user manual.

Next, I put the detector near the radioactive specimen I had purchased at the rock show. The next picture shows the pea-sized uraninite crystal enclosed in its small plastic box.

Uraninite is uranium dioxide. Over billions of years the uranium has been decaying into a number of radioactive decay products including thorium, protactinium, radium, radon, and polonium. Some of these radioactive isotopes emit beta radiation which my detector records.

When I placed the detector 18 centimeters (about 7 inches) from the encased uraninite, the detector recorded an average count rate of 38 CPM - significantly higher than background, but still safe. When I placed the detector 5 centimeters (about 2 inches) from the uraninite, however, the average count rate jumped to 726 CPM - well above the warning level! At this close position the detector was clicking like crazy and its alarm was continuously sounding!

I certainly don't want the uraninite too close to anyone for extended amounts of time. I've placed it at least 36 centimeters (about 14 inches) from any position a person might occupy, so it's in a safe place within my mineral display.

The count rates I mentioned are different than biological dose rates. Radiation dose is measured in a unit called grays. One gray is defined as one joule of radiation energy absorbed in one kilogram of matter. Different forms of radiation cause differing amounts of biological effects. For example, the biological effect of absorbing one gray of protons is about twice the effect of absorbing one gray of x-rays. The differing biological effects are incorporated into a radiation weighting factor which, when multiplied by the dose in grays, gives a biological dose unit called sieverts. Radiation dose safety limits are often stated in terms of sieverts. (Dose units are named after Louis Harold Gray (1905-1965) and Rolf Maximilian Sievert (1896-1966) who were pioneers in the measurement of radiation doses and the biological effects of those doses.)

My radiation detector, apparently, calculates biological dose rates as well as count rates. The background level around my house of approximately 20 CPM is equivalent, according to the detector, to a biological dose rate of about 0.13 microSieverts per hour. The Nuclear Regulatory Commission (NRC) recommends the general public not be exposed to rates exceeding 20 microSieverts in any one hour. My background levels are well below that threshold - less than 1/100th of the warning threshold. Even 18 centimeters (7 inches) from the uraninite the dose rate was 0.25 microSieverts per hour - still less than 1/10th the warning level for an hour of exposure. At 5 centimeters (2 inches) from the uraninite the dose rate was about 4.5 microSieverts per hour - still below the short term warning level.

For long term exposures the NRC recommends the general public not be exposed to more than one milliSievert (above background level) in a year. If my background level is 20 CPM, or 0.13 microSieverts per hour, I receive about 1.14 milliSieverts in a year just from background sources alone. I would have to double my background exposure to exceed what I understand is a very conservative safety level. 

Along with the radiation detector I also purchased a spinthariscope. It came in the colorfully labeled box shown in the next two pictures.

The principle of the spinthariscope was accidentally discovered in 1903 by William Crookes who had spilled some radioactive material containing radium on a specially prepared thin layer of zinc sulfide. When he used a magnifying glass to help pick up the spilled material, he noticed tiny flashes of light on the zinc sulfide. The light flashes were caused by impacts of individual alpha particles emitted by the radioactive material. In this way, normally invisible radiation became visible! Crookes named the device a spinthariscope by using the Greek word, spinther, meaning, spark or scintillation. This device was one of the first radiation detectors.

The next two pictures show the spinthariscope. Inside the white metal container a bit of radioactive thorium ore sits upon a moveable platform which can be raised or lowered slightly by turning the screw on the bottom of the white container. A viewing screen with zinc sulfide is located between the thorium ore and the black eyepiece at the top of the spinthariscope. The view looking down into the eyepiece is shown in the second picture below. Thorium ore emits alpha particles which hit the zinc sulfide viewing screen. The screen emits a small flash of light with each alpha particle hit.

Looking in the eyepiece.

The small light flashes are really dim. In order to see them well your eye must be completely dark adapted. This means sitting in a dark room for at least 5, 10, or 15 minutes, the longer the better. When I first looked in the eyepiece I could see flickering light that looked like small bubbles on the surface of a boiling liquid. I tried turning the eyepiece focus screw back and forth, but I couldn't get the bubbles to focus into pinpoints of light. Eventually, I tried using a magnifying glass between my eye and the eyepiece. When I did this, the result was spectacular! The viewing screen was covered with uncountable sharp speckles of light much like the magnified view of an astronomical globular star cluster filling a telescope eyepiece. Instead of constant starlight, however, the "stars" were flickering on and off. The next image of globular star cluster M5 was taken by the Hubble telescope. If you imagine all these stars rapidly winking on and off, you will get some idea of the view through the spinthariscope eyepiece.

It's amazing to see how many alpha particle bullets are continually shooting out of the radioactive ore!

Science has given us many devices that enhance and extend the senses. These radiation detectors make the invisible, visible.

Beautiful Innocence

Lovely Sisters

My good-natured little granddaughter, Annabelle, recently celebrated her 5th birthday at the Science Museum in Richmond. Her big sister, 7 year-old Sophie,  was a key participant in the festivities.

In the next picture Sophie is playing with one of the excellent interactive museum exhibits.

The museum's wonderful room for toddlers was absolutely perfect for Annabelle who is especially attracted to bright, colorful lights. She crawled in her own unique way from one exhibit to another and had a great time as you can see in the next five pictures.

After lots of play time at the museum, we went to a local cafe for lunch where Annabelle received her birthday presents.

Annabelle sat in her wheelchair while big sister Sophie helped open presents. Sophie made a special birthday card for Annabelle and read it to her.

The special card was entirely Sophie's creation. Here's the first page. (Sorry for the uneven lighting conditions.)

Here's the back of the front page:

Here's the birthday message composed entirely by Sophie:

When I heard Sophie read this, I felt like crying. There's nothing more beautiful than the honest, innocent love of a child.

Annabelle has many challenges to overcome, but sibling rivalry isn't one of them.