Category Archives: Astronomy History

1919: Hurling a Man to the Moon

1919AprPSA hundred years ago this month, the April 1919 issue of Popular Science carried this image of a hypothetical traveler to the moon. The accompanying article detailed the problems of getting there. For example, balloons or airplanes were out of the question, since they both relied upon the atmosphere for their lift. A gun was a theoretical possibility, but the article pointed out that the Earth’s escape velocity was 26,000 feet per second. But the most powerful gun at the time had a velocity of only 5500 feet per second. The article correctly predicted, however, that there was a “ray of hope in the sky-rocket.” The article reminded readers that, contrary to popular perception, a rocket did not rely upon pushing against the atmosphere. Therefore, it would work in space.

1919AprPS2Robert Goddard had already begun his experiments, but his name was not known in 1919. The only rocketeer mentioned in the article was stuntman Rodman Law, shown at left boarding a rocket for a test flight. The article notes that the flight was a spectacular failure, although Law survived. Ironically, Law died later in 1919 of tuberculosis.

It’s easy to look at an old article and laugh at the naivete of the authors.  But they got the basic concept right:  Yes, indeed, it is possible to get to the moon with rockets, and we did exactly that a half century later.  Ironically, we are once again a half century removed from being able to go to the moon.  Many readers of the 1919 article lived to see Americans walking on the moon.  Sadly, that might not be the case for readers in 2019.



1929 Communications With Mars

1929MarSciInv

Decades before the CIA teleported a young Barry Soetero to Mars, an Englishman was busy communicating with the red planet, as shown from this clipping from the March 1929 issue of Science and Invention.

Dr. Hugh Mansfield Robinson (a doctor of laws), shown standing with the headphones in the photo, had previously communicated telepathically with Mars. He followed up with a message sent by the the British Post Office radio station at Rugby (at a cost of 18 pence per word) on 18,240 meters (16.4 kHz). Since the Martians preferred 30,000 meters (10 kHz), he listened on that frequency, as shown in this picture.

Dr. Mansfield Robinson reported that he did receive a reply. Unfortunately, he was not able to translate the reply. More information is available at the BT archives.



Solar Eclipse of February 26, 1979

1979 eclipse 3.tif

1979 eclipse as seen in Bozeman, Montana. Wikipedia photo.

Today marks the 40th anniversary of the solar eclipse of February 26, 1979.  The path of totality passed through Washington, Oregon, Idaho, Montana, and North Dakota before entering Saskatchewan, Manitoba, Ontario, Quebec, and the Northwest Territories. From Canada, the path of totality entered the north Atlantic before ending in Greenland.

The path through Winnipeg, Manitoba, was tantalizingly close to my home in Minnesota, but I was unable to travel to see the spectacle. I had to settle for 90% coverage (in other words, millions of times more sunlight) where I was. I did vow that I would see the next one, in 2017, and I did.

This video shows coverage of the eclipse as totality passed through Winnipeg:



Lunar Eclipse, January 20, 2019

While not nearly as spectacular as a solar eclipse, another interesting astronomical phenomenon will be visible this Sunday evening throughout the Western Hemisphere.  This will be a lunar eclipse, in which the moon passes through the shadow of the earth.

The eclipse begins at 9:36 PM Eastern Time (8:36 CST, 7:36 MST, 6:36 PST) with the penumbral phase, as the moon enters the outer shadow of the earth. The brightness of the moon will decrease, but the small change in brightness probably won’t be visible to the naked eye.

About an hour later at 10:33 PM Eastern Time (9:33 CST, 8:33 MST, 7:33 PST), the eclipse enters the partial stage. At this time, the earth’s shadow begins to eat away at the moon. This continues until 11:41 PM Eastern Time (10:41 CST, 9:41 MST, 8:41 PST), when the eclipse becomes full, and the moon is completely within the shadow of the earth.

Unlike a solar eclipse, the times are more or less identical wherever you are.  You only need to adjust for your time zone.

Image result for lunar eclipse site:nasa.govEven though the eclipse is full, the moon does not become fully dark. This is because the moon is illuminated by a ring surrounding the earth, namely, all of the sunrises and sunsets taking place on earth.

At 12:43 AM Eastern Time, the eclipse once again becomes partial. At 1:50 AM Eastern Time, it re-enters the penumbral phase. At 2:48 AM Eastern Time, the eclipse ends.

We previously wrote of an interesting story of a lunar eclipse of July 15, 1916. This eclipse affected the Shackleton Antarctic expedition. The team led by Aeneas Mackintosh was waiting for a full moon to embark, but were surprised to see the moon entering an eclipse as it rose. Fortunately, the eclipse was only partial and enough light remained to make the voyage.



NBC Radio, Canton Island Eclipse Coverage, 1937

1938Sep5LifeThis picture appeared in an RCA advertisement in Life magazine 80 years ago today, September 5, 1938. It shows NBC engineers Marvyn Adams and W.R. Brown along with NBC announcer George Hicks broadcasting live from Canton Island (sometimes spelled Kanton) in the South Pacific.

1937 Eclipse from Canton Island. Wikipedia image.

They were on the island as part of a joint expedition by the U.S. Navy and the  National Geographic Society for the solar eclipse of June 8, 1937.  The NBC eclipse coverage was transmitted from this “ultra-high frequency transmitter” to the USS Avocet anchored at the island, and from there to the RCA station at Point Reyes, California, where it went by wire to the NBC Blue Network.

According to the ad, the island would possibly “play an important role in transpacific air transport service,” a prophecy which proved true, as the island served as a stop for PanAm’s Pacific Clipper service to New Zealand, which ran from 1940 until the war, and then again from 1946.

The Navy-National Geographic expedition, in addition to observing the eclipse, placed a monument on the island to bolster the U.S. claim to sovereignty over the island. This was disputed by the British, who also had a ship anchored for the eclipse. Reportedly, the British ship, the HMS Wellington, fired a shot across the bow of the USS Avocet, which reciprocated. The two commanders called a truce pending further instructions from their command, and the two parties observed the eclipse together.

During the war, the U.S. Navy built a 6230 foot airstrip on the island, which was defended by as many as 1200 combat forces, but was never attacked by Japan.  The island now forms part of the Republic of Kiribati.  As of 2010, it had a population of 24.

The island was most recently in the news that year after a yacht stopped en route from Honolulu to Fiji and discovered that the islanders were desperately short of food, an expected supply ship never having arrived.  The islanders had been living on fish and coconuts for several months, and the yacht owner used his satellite phone to contact the U.K. Coast Guard, which contacted the U.S. Coast Guard to arrange relief supplies.



More Planning Advice for Time Travelers

Admittedly it’s unlikely that you’ll need the information, but we occasionally provide useful advice to keep in mind in case you’re ever inadvertently subjected to time travel. If you get caught in a time warp, the experience will be much less unpleasant if you do some minimal preparation.

For example, if you get sent back to the past, your situation would be much improved if you could “invent” some modern technology. Columbus could use some better navigational tools to determine that he had not, in fact, reached India.  Louis XVI would have been more likely to keep his head with a telegraph to better manage the affairs of his kingdom.  Just about wherever and whenever you arrive, you’ll have similar opportunities involving people who would be willing to pay handsomely for bits of technology that you can invent.

We’ve previously written about the importance of having a WikiReader, which holds the contents of the English Wikipedia in a handheld device.  And we’ve written about how to make the most difficult component of a radio receiver, the earphone, from scratch.

We’re confident that most of our readers will do well if they’re ever whisked back into time.

How to Figure Out the Date

In many situations, you’ll be able to determine the date easily.  If you’re in an urban area in the past few centuries, you can simply peek at a newspaper.  You can even  ask people on the street what year it is.  They might give you a funny look, but if more than one person gives you the same answer, it’s a safe bet that they’re telling the truth.  If they’re not clear on the concept of the A.D. scale, then you can determine things such as the name of the king, and use your WikiReader to figure out the year.

But in some cases, this information might not be quite so convenient.  Fortunately, the night sky provides a convenient clock, and with a bit of number crunching, you should be able to figure out the date.

Determining the Day of the Year

The first step is to determine the day of the year, and this is quite easy.  You simply observe the local sunrise and sunset times.  The sunrise and sunset times will be the same from year to year, so you can use a reference for any year.  Just note the time of sunrise and sunset, and see which day they correspond with.  You’ll probably come up with two possible dates, so you might need to check again to see whether the days are getting longer or shorter.  In the Northern Hemisphere, if the days are getting longer, then the date is after December 21 but before June 21.  If the days are getting shorter, then it’s after June 21 but before December 21.  The best source of sunrise and sunset times is probably the Old Farmer’s Almanac, although this information should be available in many places.  You can probably find it somewhere on your WikiReader.  Remember, the year of your source is unimportant, since the data will be about the same from year to year.

Determining the Year

The planets. NASA image.

The planets. NASA image.

Now that you know the month and day, you can move to the next step, namely, figuring out what year it is.  For this, you can use the planets.  The planets Mercury, Venus, Mars, Jupiter, and Saturn are all visible to the naked eye.  On any given date, each one of them is supposed to be in a particular spot in the sky, in one of the twelve constellations of the zodiac.   You start by finding these planets and noting what constellation they are in.

At this point, you can go to a website such as Your Sky, start punching in the various possible dates, and see which one corresponds to the observed data.  When you get a match, you know the exact date, at least within a few days.  For example, currently (1 August 2018), Mercury is in Cancer, Venus is halfway between Leo and Virgo, Mars is right between Capricorn and Sagittarius, Jupiter is in Libra, and Saturn is between Scorpio and Sagittarius.

So if I knew it was August 1, I would simply use that date, and repeat the process with different years until I found that the planets matched up with what I was seeing in the sky.  In this case, as soon as I plugged in 2018, I would see that it matched, and know that I guessed the year correctly.

How To Do This Without the Internet

Of course, I’m sure that by now you’ve spotted a big flaw in this strategy.  If you have the internet available, then you can just ask the internet what date it is.  But that website, and others like it, merely employ a relatively simple computer program.  You can find all of the information you need to calculate the same positions by using a book such as Practical Astronomy With Your Calculator or Spreadsheet.  It will contain all of the information you need to do the calculations, either with a calculator or computer, or if all else fails, with pencil and paper.  You can buy the book now, before the time warp.

On the other hand, you’re probably thinking that the likelihood of needing such a book is quite small.  If you don’t get stuck in a time warp, then it’s money wasted, and I would have a hard time arguing with you.  In fact, if you get sent back along with a public library, you’ll probably be able to find a similar book there.

You'll want to use the full size version of this chart, which is available, along with complete instructions, at this link.

You’ll want to use the full size version of this chart, which is available, along with complete instructions, at this link.

But there’s still a minimal level of preparation with practically zero cost!  I found this homework assignment from a college astronomy course.  If you print this out before getting sent back in time, it actually includes all the information you will need to calculate the positions of the five visible planets!  It uses a graphical method:  Right there on the worksheet it gives the position of the planets as of a certain date.  You simply calculate how many times each planet will need to go around to reach that date.  After you do the division, the remainder is the portion of one orbit the planet is away from that spot.  You plot the position of both that planet and the Earth on the provided graph, and you can then see where in the sky the planet is located on a given date.

This method is not as precise as the computer programs, but those computer programs are designed to show you exactly where to point your telescope.  You don’t need that level of precision.  By graphing the general location of several planets, you will be able to confirm what year it is.

You should download (or better yet, print) that worksheet now, before the time warp.

Checking Your Work

PrecessionOfEquinoxesTo confirm that you’ve picked the correct year, you might want to use another method.  It’s possible, for example, that all of the planets were in the same position in the sky on today’s date millions of years ago.  The best way to check your work is to use the precession of the equinoxes.  Simply put, the star Polaris is currently located at the North Celestial Pole.  In other words, all of the stars in the sky seem to revolve around this point.  But the celestial pole moves over time, following a 26,000 year cycle.   You’ll want to print the handy chart shown here.  Match up the pole star with the chart, and you’ll know where you are in the cycle.  For example, if you discover that Vega is the pole star, that means the year is approximately 11,000 BC (or maybe 12,000 AD).



1952 and 1954 Solar Eclipses

SovietEclipseCoverMillions of Americans were able to witness the Great American Eclipse of 2017 or will be able  to see the eclipse of April 8, 2024.  The 2017 eclipse crossed the United States from northwest to southeast, and the 2024 eclipse will run from southwest to northeast.  The Soviet Union had a similar pair of eclipses on 25 February 1952 and 30 June 1954.  The intersection of the two American eclipses is near Carbondale, Illinois.  The paths of the two Soviet eclipses had their intersection at a point in northern Iran, just south of the Caspian Sea.

SovietEclipseMap

The illustrations shown here are from a Soviet booklet published in 1950.  In addition to discussing solar and lunar eclipses generally, it contains information about the two Soviet eclipses of the 1950’s, including the map shown above.  It also contains a table showing all total solar eclipses worldwide through 1999.

The booklet, Солнечные и лунные затмения (Solar and Lunar Eclipses) by Prof. A.A. Mikhailov, part of the series Научно-популярная библиотека (Popular science library), reveals that the path of the 1954 eclipse came very close to a number of Soviet cities, including Kaliningrad, Vilnius, Minsk, Kiev, Rostov, and Baku.   The 1954 eclipse had also been visible in the United States, starting at sunrise in Nebraska, and passing over South Dakota and Minnesota (including Minneapolis and St. Paul).  It then passed over Canada, Greenland, a tiny portion of Iceland, Norway, and Sweden, before entering the Soviet Union near Kaliningrad.

The 1952 eclipse, after passing over Africa, went over a less populated area of Turkmenistan, Uzbekistan, Kazakhstan, and Asiatic Russia.

This video shows the 1954 eclipse from Minneapolis:

This page contains a reminiscence and photo of the same eclipse from Kiev.  The Google translate function does an admirable job of making it readable in English.

One of the scientific observations made during the 1954 eclipse was the measurement of radio emissions by the sun on various frequencies, documented in this 1955 article in the journal Astrophisica Norvegica, vol. 5, p. 131.  The graph below shows the signal as received in Vesterøya, Norway, on 200 MHz.  As would be expected, the solar noise reaches a minimum value at the time of total eclipse.

1954EclipseRadio

Information on how to form a Minnesota LLC.



Laika’s Flight: November 3, 1957

On this day 60 years ago, November 3, 1957, Laika, a Soviet dog, became the first Earth creature to orbit the Earth.

Her survival was never expected, since the technology to de-orbit had not yet been developed. Little was known about the impact of spaceflight on living creatures, and some scientists believed that it would be impossible to survive the launch. Laika’s mission was designed to determine whether a living creature could survive the forces of launch and the micro-g environment of space travel.

The Soviets initially claimed that Laika was humanely euthanised by lack of oxygen. However, her actual cause of death was made public in 2002, when it was revealed that the spacecraft overheated, causing her death within a few hours.

Laika was originally a stray found wandering the streets of Moscow. It was thought that such animals were already well adapted to surivial. Three dogs were trained, and Laika was finally selected as the “lucky” winner to make the one-way trip to the final frontier. She was trained by being kept in progressively smaller cages. Before the launch, one scientist took Laika home to play with his children. He reported, “Laika was quiet and charming. I wanted to do something nice for her. She had so little time left to live.”

She was hooked to sensors, and on November 3, 1957, she was launched on her mission from the Baikonur Cosmodrome. When a piece of thermal insulation tore loose, the temperature of the capsule soon reached about 104 °F. Laika died of overheating on about the fourth orbit.

After 2570 orbits, the Sputnik 2 spacecraft, along with Laika’s remains, disintegrated during re-entry on April 14, 1958.


Calibrating Your Watch With The Stars

1947OctPSSeventy years ago, the October 1947 issue of Popular Science showed this method of making sure your watch was accurate.

While this method would not, by itself, give you the exact time, it would very precisely tell you the elapsed time.

The method was very simple. You simply installed a piece of tin with 1/16 inch hole on some fixed location, such as the side of the building. You used it to sight a vertical fixed object, such as a lightning rod or distant skyscraper. Then, you observed the exact time that any star was occluded by the object. Since the star is essentially a point of light, it would disappear suddenly. You noted the time.

Then, the next evening, you would observe the same star. It would be occluded exactly 23 hours, 56 minutes, 4.09 seconds later–one sidereal day. In other words, the time on your watch should read exactly 3 minutes 55.91 seconds before the previous night’s figure.  (For all practical purposes, a sidereal day is 364/365 of a solar day.  This makes sense, since the Earth itself has moved 1/365 of its way around the sun in 24 hours.)

Depending on whether your watch was fast or slow, you could thus adjust the spring.

If you knew the exact time the first night, then you could also create a table showing the exact time of occlusion subsequent nights. As long as you didn’t move the piece of tin, you would always know what time it is.

This method has two applications.  After the zombie apocalypse, presumably WWV will be off the air.  The stars give you a method to keep your clock calibrated very accurately.  It could also be the basis for a very interesting science fair project.

 

 



Sputnik: October 4, 1957

Sixty years ago today, the Space Age started when the Soviet Union stunned the world by launching Sputnik 1, the Earth’s first artificial satellite, on October 4, 1957.

Soviet news agency TASS made the official announcement:

As a result of very intensive work by scientific research institutes and design bureaus the first artificial satellite in the world has been created. On October 4, 1957, this first satellite was successfully launched in the USSR. According to preliminary data, the carrier rocket has imparted to the satellite the required orbital velocity of about 8000 meters per second. At the present time the satellite is describing elliptical trajectories around the earth, and its flight can be observed in the rays of the rising and setting sun with the aid of very simple optical instruments (binoculars, telescopes, etc.).

In addition to reminding the West that the satellite could be seen by anyone, TASS went out of its way to make sure that even radio amateurs could hear for themselves that the Soviets had won the race into space.  The official press release included Sputnik’s frequencies:

 It is equipped with two radio transmitters continuously emitting signals at frequencies of 20.005 and 40.002 megacycles per second (wave lengths of about 15 and 7.5 meters, respectively). The power of the transmitters ensures reliable reception of the signals by a broad range of radio amateurs. The signals have the form of telegraph pulses of about 0.3 second’s duration with a  pause of the same duration. The signal of one frequency is sent during the pause in the signal of the other frequency.

Sputnik 1.jpg

Replica of Sputnik 1. Wikipedia photo.

Receivers for the 40 MHz signal would have been a rarity, but thousands of hams and SWL’s had receivers that would easily tune 20 MHz.  The frequency was cleverly picked to be close to WWV’s powerful 20 MHz signal.  Thus, even though most receivers weren’t calibrated well enough to show the exact frequency, the U.S. National Bureau of Standards unwittingly made sure that everyone knew exactly where to tune.

In addition, the signal was so close to WWV, then at Beltsville, Maryland, that the unmodulated carrier from the satellite would create a heterodyne with WWV, allowing it to be heard even if the receiver was a simple one without a BFO.

The national association of amateur radio operators, ARRL, was flooded with calls from reporters.  They gave instructions to listeners to “tune in 20 megacycles sharply, by the time signals, given on that frequency. Then tune to slightly higher frequencies. The ‘beep, beep’ sound of the satellite can be heard each time it rounds the globe.”

1957DecQSTThe December 1957 issue of QST included several photos of hams who had heard the satellite,  And in many cases, those hams made the signal available to local broadcast stations and news outlets.

In Chicago, it was 27-year-old ham Jerome Tannenbaum, W9JJN, of 5240 Harper Avenue. He was described in the October 5 Chicago Tribune as the owner of an electronic engineering consulting firm and radio operator since he was 15. He told the newspaper that he heard a steady stream of “dahs” on 20.005, and definitely believed that the signal was from Sputnik, based upon the fact that it faded out right when predicted.

Hams quickly figured out how to track the orbit and predict the next time the satellite would be in range.  Again, Moscow made sure they knew Sputnik’s orbital inclination of 65 degrees,  and orbital period of 1 hour 35 minutes, by including this information in the first announcement.  The simple locating device shown here was made at ARRL headquarters, merely by mounting a loop of wire around a globe.  Once the satellite was heard, it was a simple matter of predicting where it would be heard next by rotating the Earth 23.75 degrees, the amount it would move during one orbit.

Apparently, Sputnik had at least one deliberate QRM’er.  A letter in the December 1957 issue of QST reports that someone showed up on 20.005 MHz on October 7 with commentary such as, “this is the moon speaking,” sending the safety signal, and signing the call sign UA3ABD.  The letter writer, Dave Harris, K2RRH of Lyndhurst, N.J., hoped “that donkey realizes that he is on tapes all across the country.”

Sputnik 1 remained in orbit until January 4, 1958, having completed 1440 orbits of the Earth.  When it re-entered the atmosphere, WWV played another role.  Hams and others were already familiar with meteor scatter, the reflection of radio signals by the ionized gasses caused when a meteor enters the atmosphere.  Scientists and hams correctly guessed that Sputnik would cause the same phenomenon on re-entry.  As a convenient signal source, WWV was once again used, and as predicted, the WWV signal appeared or got louder as the satellite entered the atmosphere.  With this data, it was possible to track the satellite’s location until it completely disintegrated in the atmosphere.

Thousands of Americans were able to see or hear Sputnik.  In many cases, this sparked a lifelong interest in science, space, and/or radio.  I asked some of the hams at QRZ.com to share there stories about their experiences.  A number of hams posted there or e-mailed their recollections.

Glen Zook, K9STH, currently of Richardson, Texas, shared this story of hearing Sputnik as a 13 year old in LaPorte, Indiana, and he gave me permission to include it here:

Hallicrafters S-40

Hallicrafters S-40

There was a garage shop TV repair facility about a block south of my parents’ house. When Sputnik was launched and was operating, the frequency, 20.005 MHz, and the expected times when the satellite could be heard, were published in the LaPorte Herald Argus newspaper. Orville Hartle, the owner of the TV shop, had a Hallicrafters S-40 receiver and invited my father to come down and listen to Sputnik. I “tagged along” with my father.

As the expected time for the satellite to become in range, Orville started “fiddling” with the receiver. Nothing was heard! Finally, the “beep, beep, beep” from the satellite’s transmitter came faintly from the S-40’s receiver. Today, such a happening would be “ho hum”. However, in 1957 this was very exciting if, for no other reason, that the signal could be received by “Joe Blow” and not just by a very sophisticated scientific or military installation.

The repercussions from this evening, at least in my personal life, were great. Orville discovered that I had a serious interest in electronics which his son, who was about a year younger than I, had absolutely no interest. In fact, his son had very little interest in anything! Orville was an unusual character! He was a graduate EE but worked in the “tool crib” at the local Allis Chalmers plant, ran the TV shop evenings and weekends, and wrote books!

Orville started giving me as many old television chassis that I could “haul off” for the purpose of stripping for parts. I would take my sister’s “little red wagon” (she is 7-years younger than I) down to the TV shop and Orville would put 2, or 3, chassis in the wagon and I would bring them to my house. There were outside stairs to the basement and I would carry the chassis down and put them next to a workbench that my father had built next to the coal bin. My “experiments” were conducted, primarily, on that bench.

Thinking back, I cannot help but believe that Orville was a contributing factor to the fact that for Christmas, 1957, my parents bought me a used Heath AR-3 receiver (from Allied Radio Company in Chicago). Prior to that Christmas, I had been using an old TrueTone (Western Auto private brand) receiver with a shortwave band.

He was not an amateur radio operator, but he did encourage me to experiment with electronics and even gave me a television set, for my room, that was better than the one in my parent’s living room!

With the help of Dave Osborn, K9BPV, I passed my Novice Class examinations on my 15th birthday, 13 February 1959. It took over 3-months for the license to arrive in the mail. The license is dated 15 May 1959 but took an additional almost 2-weeks to come in the mail. I was just ending my freshman year in high school. In October, I took my General Class examinations at the FCC office in Chicago.

Then, in August 1962, between my senior year in high school and my freshman year in college, I took the examinations for my commercial radiotelephone operator’s license. My junior year at Georgia Tech, I got married and also got a job at the Motorola Service Station in Atlanta, Georgia. My senior year, I was hired directly by Motorola to establish, and then manage, the first Motorola owned portable / pager repair facility away from the Schamburg, Illinois, plant. After graduating, I was employed by the Collins Radio Company at the “new” corporate headquarters here in Richardson, Texas, and the “rest is history”!

All of this starting with the listening to Sputnik in October 1957!

Jim Allen, W6OGC, of New Braunfels, Texas, sent this account, which I share with his permission:

Sputnik went up in October, 1957, and lasted something like 3 months

One evening as we sat eating supper, the telephone rang. My dad got up and answered. He recognized the caller, the Superintendent of Schools, then became as flustered as I ever saw him. “Why, yes, he’s here. I’ll get him.”

He gestured to me, I got up and answered the phone. My dad hovered around with a look in his face, “there better be a heck of a good story for this!” He could not imagine why this big shot was calling for me, a 6th grader.

Hallicrafters SX-100. Radio News, ______.

Hallicrafters SX-100. Radio News, Feb. 1956.

The Super, W5FFE, said to me, “listen to this.” I heard the beep, beep, beep, that no one had ever heard before. He explained it was a satellite, the first one, and he was listening to it on his radio, an SX-100 as I knew. I had been watching the launches from Florida, none successful thus far.

A few of us had been going to Novice classes, he knew of it, and had called some of us, each pass.

I don’t think my dad ever forgot that.

One surprise for me was the number of hams (and other members of the public) who saw Sputnik with their eyes.  A number of such reminiscences were posted, although many of the viewers realized years later that they probably hadn’t seen Sputnik itself, but rather the larger covers that had been jettisoned from the smaller satellite.   But still, they were watching with their own eyes something the Soviets had put into orbit.

It shouldn’t have come as a surprise that so many people saw Sputnik (or the other parts of the spacecraft).  Today, when randomly stargazing, it’s not uncommon to see an artificial satellite cross the sky.  After all, there are thousands of them, and just by randomly looking up, you’re bound to eventually see one.  In fact, it’s almost mundane.  When I was growing up in the mid-sixties, it wasn’t uncommon for my parents to point one out to me.  It was already mundane, but there they were for all the world to see.  It did strike me as amazing.

I remember reading about the Lykov family, who, starting in 1936, lived in complete isolation from society in Siberia for 42 years.  According to one account,  They had noticed starting in the 1950’s that “the stars began to go quickly across the sky.” The father, Karp Lykov, surmised that “people have thought something up and are sending out fires that are very like stars.”

When Sputnik 1 went up, it wasn’t mundane, and the predicted times of orbits were published in newspapers.  Millions of people were looking up, expecting it.  It shouldn’t have surprised me that so many of them still remember.