A Stellar Life

1

CRATER ELEGANTE

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ne Christmas vacation Bill Miller and I decided to search for the remains of the Camino del Diablo (Highway of Death) in his jeep. That was the dirt road along the Arizona-Mexico border that some of the ‘49ers used to avoid the mountains farther north in going to the gold rush in California. There was little water along the road, only the natural spring at Quitobaquito Spring (Fig. 1-1) in what is now Organ Pipe National Monument and in the natural tanks in the Tinajas Altos Mts. After rains, water remained in the stone pockets in the latter, but one had to climb up to them. Skeletons farther down showed the people who did not have the strength to climb up. The Quitobaquito Spring has been in the news recently because of the evidence that this rare oasis in the Sonora Desert is now in danger of drying up due in part to the fence being built along the border. It cuts through the Tohono O’odham Reservation. The fence divides families, as did the Berlin Wall, and the passage of animals.

The Arizona Highways had just come out with an article about people who had found a way to climb down to the bottom of Crater Elegante (Fig. 1-2) in the Pinacate crater region, now called the Pinacate National Park in Mexico. We drove to that crater. Bill wondered if it was of meteoric or volcanic origin. Several months later he organized an expedition to it with Caltech Geologist Robert Sharp, USC meteor expert Frederick Leonard, Caltech student Barclay Kamb, Bill, and I. Barclay later was a geologist and Provost at Caltech and married Linus Pauling's daughter.

Fig. 1-1: The Quitobaquito Spring in Pipe Springs National Monument, a natural oasis in the Sonoran Desert just north of the Arizona-Mexico border.

The crater is 1.5 km across and 250 m (820’) deep. We climbed to the bottom. Dr. Leonard found no meteoric material in or around it. Dr. Sharp called it a collapsed caldera, in which water seeping down encounters hot magna that produces a huge explosion, throwing rocks up to 19 km away. More recently that explosion has been dated as 32,000 years ago.

Fig. 1-2. Carter Elegante in Pinacate National Park in Mexico, just off the road to Rocky Point (Punta Penasco).

2

THE CRAB NEBULA SUPERNOVA

Fig. 2-1. A Hubble picture of the Crab Nebula. The red features are due to HΑ radiation from the gaseous filaments. The central blue light is synchrotron radiation coming from the pulsar at the center.

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he Crab Nebula (Messier 1) is a beautiful gaseous nebula (Fig. 2-1) in Taurus which is the result of a supernova that exploded in 1054 AD. The Chinese astronomers kept records of guest, or new, stars because they thought that they affected people, i.e. astrology. A Swedish astronomer (Lundmark 1921) collected 60 such records between 134 BC and 1828 AD. No. 36 in his list occurred in Taurus in 1054 AD and the Chinese position agreed with the position of the Crab Nebula.

Astronomers Lampland (1921) at the Lowell Obs. and Duncan (1921) at the Steward Obs. found that the Crab Nebula is expanding and Hubble (1928) suggested that the Crab Nebula is the remnant of that explosion. Duncan (Mayall & Oort 1942), Deutsch & Lavdovsky (1940) and Trimble (1968) derived explosion dates in the 12th century, but those are valid for only the radial motion of that turbulent nebula. The Chinese first saw the explosion on 5 July 1054 (Clark & Stephenson 1977). They said that it was visible in daylight for 26 days and at night for 653 days.

The Japanese (Duyvendak 1942) also recorded the bright star but their date in the summer of 1054 AD was uncertain.

In June 1953 Bill Miller and I explored the top of White Mesa for three weeks. It is a 180 m (600 ft.) high mesa (Fig. 2-2) on the Navajo Reservation in northern Arizona, northeast of Tuba City.

Fig. 2-2. In the background is White Mesa as seen from US160 at the bottom. Only Navahos are allowed to leave the highway; the Navaho police effectively keep pot-hunters off the reservation. (Photo by the author.)

He had obtained permission to explore the 25 km² top from the Navajo Council because it had never been explored by an archeologist, according to the Museum of Northern Arizona staff in Flagstaff. Potsherds told Bill that it had been inhabited in the 10-13th centuries, but not since. Among the thousands of pictographs he found one of a crescent moon next to a circle, the latter indicating something big or bright (Fig. 2-3). He knew that the Native Americans rarely showed anything astronomical. He wondered whether it was a drawing of an eclipse, which was not so rare as to cause them to draw it? Fred Hoyle (in residence in Pasadena at the time) suggested it might represent the Crab Nebula Supernova. With help from Walter Baade, Bill computed, using Brown's lunar tables, that on 5 July 1054 the new star was within 2 deg. of the Moon and it was in a crescent phase.

The next year Bill and I explored the lower part of Navajo Canyon on a governmental grant because it would be flooded by Lake Powell after Glen Canyon Dam was completed. In the upper part of the canyon I found a similar pictograph, but it was a reflection of the one on White Mesa (Fig. 2-4). Bill published (Miller 1955) a description of these.

Brandt & Williamson (1979) wrote to National Park Superintendents in the American southwest as to whether they had seen similar pictographs. Together with Mayer (1979) and Fountain (2000), 31 more were found, roughly divided between the ones in Figures 2-3 and 2-4.

Fig. 2-3. The Crab Nebula supernova pictograph that Bill Miller found on White Mesa. It is a drawing on the sandstone walls of a cave. It represents what one would see in the spring of 1054 AD. (Photo by the late Bill Miller)

Fig. 2-4. The supernova pictograph I found in Navaho Canyon. It represents what one would see in the summer of 1054 AD. (Photo by the author.)

But was the supernova seen elsewhere? Collins et al. (1999) made a search of European and near eastern ecclesiastical records from the 11th and later centuries. They found seven accounts of a new bright star seen between 11 April and 20 May 1054 in the evening (and daylight!) sky before the Crab Nebula went into conjunction behind the Sun.

This leaves two dilemmas: why did the Asians not record the bright star in the spring before it went into conjunction behind the Sun and why did the Europeans not record the bright star in the summer after it came out of conjunction? We have only guesses, but they seem to make sense.

The Chinese astronomers undoubtedly saw the supernova in the spring, but in China at that time it was thought that an extremely bright guest star meant that the Emperor would die or that there would be a new dynasty. Telling the Emperor that he would probably die soon would be lethal for the astronomers, especially because the Emperor's favorite concubine had just died and he was in a depressed mood. The astronomers knew that the guest star would soon disappear behind the Sun, so maybe if they waited, it might not be there in the summer. They waited, but it was there in July and they had to report it. We do not know what happened to the astronomers, but the Emperor died the next year.

Why did the European church documents report the bright star in the spring of 1054 but not in the summer? That was the year when there was a serious effort to combine the Roman Catholic Church and the Eastern Orthodox Church. They worked on a plan for nearly a year, but announced on 16 July that they had failed. It is called the Eastern Schism. But there in the sky was a new bright star that could be seen in the daytime! Was that God's condemnation of their failed efforts? It might have been safer to the record keepers not to record the bright star in the summer.

However, the Native Americans evidently saw the supernova both in the spring and summer of 1054; that is why they drew it in the spring, like the Navajo Canyon pictograph, and in the summer, like the White Mesa pictograph.

There are still problems in understanding the type of supernova this was because none of the recent ones stay near maximum light for 80 days. We are learning that supernovae are more complicated and individual than we previously thought. Part of the above was published in Abt & Fountain (2018) in a Chinese publication.

3

INTRODUCTION

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am not writing this book because I think that people in the future will be interested in me. I never received any major awards or prizes and will be forgotten in several decades. I started some new areas of astronomy, but others later will repeat that work with better data and my early contributions will be forgotten. Instead, consider me as a wallflower who witnessed the rapid growth of astrophysics during the 20th century and knew many of the participants. I initiated new policies and technologies in publications, such as making the ApJ more international in content and participation, and converting to digital operation and publication. I will shock some people who still think that religious organizations should determine how people should live, as they did in 15th century Europe and where slavery was allowed. I visited places that later became overrun with tourists. I hope that you will find the following interesting after a few words of introduction.

My foster son, Daniel V. Conaway, suggested the title of this book and helped me reorganize it. Mike Peralta solved some major computing problems for me.

My family came to the US in 1927 after my father lost his furniture factory during the German inflation. I was two years old at that time. In the rapid inflation when the value of the money changed twice daily, people could not save up to bury furniture. Also laws prevented employers from laying off employees. My father set up as a furniture designer in the US, favoring the Bauhaus modern style while most Americams favored the colonial style. We lived in Jamestown, NY, the furniture capital of the country at the time.

Jamestown was the home of three famous people. One was Roger Tory Peterson (1908-1996), who published the first modern Guide to the Birds, which sold out in one week. He published six later editions. There is a Roger Tory Peterson Institute in Jamestown.

The second famous person from Jamestown was Lucille Ball, a comedienne who became famous later for I Love Lucy on TV. There is a museum in Jamestown of her memorabilia.

The third famous person from Jamestown was Robert H. Jackson. He was a legal advisor to Franklin D. Roosevelt while the latter was Governor of NY. After Roosevelt became President, he appointed Jackson as General Counsel for the IRS, then US Solicitor General, then US Attorney General (1940-41), and then Associate Justice of the US Supreme Court (1941-1954). At the end of WWII Pres. Truman appointed him as the Chief Prosecutor at the Nuremberg trial of Nazi leaders. He returned to the Supreme Court in 1946 but died of heart problems in 1954. There is an active Robert H. Jackson Institute in Jamestown. In 1939 I worked after school in the massage facility in the YMCA. I changed sheets, cleaned up messes, ran errands, etc. When Jackson came in, my Hispanic boss whispered to me that he was a famous lawyer. I remember Jackson as being thin, of moderate height, dark hair, and reserved.

My mother was an excellent pianist and I remember her playing the Schubert Impromptus. Her teacher in Jamestown was Mrs. Appisch, a pupil of Egan Petri, who was known for his beautiful touch. Petri was a pupil of Ferruccio Busoni and, in turn, Petri became the teacher of many famous pianists such Victor Borge, Eugene Istomin, Gunnar Johansen, Ozan Marsh, John Ogdon, and Earl Wild.

4

HIGH SCHOOL AND UNIVERSITY IN ILLINOIS (1940-1948)

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s the furniture business in Jamestown gradually failed, my family moved to the Chicago area where my father worked for Storkline, a baby furniture company. Even in a depression new parents need furniture for a baby and are unlikely to settle for used furniture. My father died suddenly of a heart attack in 1940, leaving my mother, who had never worked for a living, to raise my brother (17) and me (15).

As a high-school student in Oak Park, IL and facing the WWII draft, I realized that I would just become a soldier unless I was in a university and qualified for a higher position. My brother Karl was a university student with language experience. In the army he helped interview captured German soldiers. They abided by international standards, asking only name, rank, and serial number. But some German soldiers were disgusted with the Nazis. His group learned that the Germans were amassing a million troops in the Netherlands for a last stand and it sent that information to the Allied headquarters. The info was ignored – hence the Battle of the Bulge where thousands of Allied troops were killed (Abt, K. 2004).

I arranged to pass my senior year courses by exam and entered Northwestern Univ. a half-year before my high school graduation. At Northwestern I majored in math because I was unsure where I was headed, and soon obtained part-time employment by grading homework papers for math courses. Later I ran physics labs, obtained x-ray diffraction pictures for chemists, and tested aircraft rivets for an engineering professor. I failed the draft for a trivial reason – a pilonidal cyst, which had been cured. I soon shifted to physics and my M.S. thesis advisor was Dr. Russell A. Fisher.

Dr. Fisher had an interesting time during WWII. He was a member of the ALSOS Mission. The US wondered whether the Germans were working on an atomic bomb. The mission consisted of military, scientific, and intelligence personnel. The head was Brigadier General Leslie Groves (alsos is the Greek word for grove), who later wrote a book about the mission. Dr. Samuel Goudsmit was the Chief Scientific Advisor. He had not worked for the Manhattan Project, so if captured by the Germans, he could not be forced to reveal any American secrets. He had 33 scientists working with him. One was Dr. Russell Fisher.

Goudsmit had been on the University of Michigan faculty, where he and George E. Uhlenbeck in 1925 proposed that electrons have spins. He was Jewish and born in the Netherlands. His parents were killed by the Nazis in 1943. Later Goudsmit headed the Physics Dept. at NU (1948-70), was at the Brookhaven National Lab. (1952-60), and was Editor-in-Chief of the Physical Review (1950-74). He started the Physical Review Letters.

The ALSOS scientists reasoned that if the Germans were working on an atomic bomb anywhere is western Germany, some radioactivity would get into the Rhine River water. So during the Battle of the Bulge, they had Fisher crawl half way across a bridge over the Rhine under bombardment and lower bottles to collect samples of the water. They had no way to test the water, so they sent the three bottles to Washington, DC for testing. Because the bottles would rattle in the box they had, they added a bottle of French wine with a joking label Test this for radioactivity too. The reply came back No radioactivity in the Rhine River water, but there is in the French wine. Send more wine! The ALSOS scientists felt that the people in Washington just wanted French wine, and ignored the request. But the request went up the official chain until they could not ignore it. In some places the soil is naturally radioactive, so they sent Fisher to southern France from where the wine came. Fisher collected samples of the soils, water, grapes, and wines, and sent them all to Washington. No further requests.

Although physics, especially spectroscopy, was fun, a course in astrophysics taught by Wasley S. Krogdahl using Goldberg & Aller's book really turned me on. I received admittance from Princeton but they specialized in theoretical studies. The University of Chicago also would accept me but had no available student financial support. However I learned at Yerkes Observatory from Drs. Struve, Kuiper, and Greenstein that Caltech was going to start an Astronomy Dept. in the fall of 1948, just after the Palomar 200-inch (5.1m) was dedicated. I applied and received acceptance and an assistantship.

5

CALTECH (1948-1952)

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n August 1948 I took the Sante Fe train from Chicago to Pasadena (38 hours). I had shipped my bike ahead to the Pasadena YMCA and arranged to stay there. My Assistantship paid $100 per month and I doubted that I could live on that amount. I went to the Caltech housing office to find out what housing was available. It had an offer from a local doctor and his wife (Dr. John and Virginia Bolenbaugh) for a free room to a Caltech student in exchange for baby-sitting for their two boys, Andy (6) and Rich (4), three or four nights a week. Their house (3575 San Pasqual St.) was at the east end of Pasadena, three miles from Caltech, but that was OK on a bike because it seldom rained there.

I rode there and met Virginia and the boys, and we liked each other. However Virginia said that I should first get the approval from her husband at his office on Hill St. He agreed, but was amused that Virginia had already given me a house key!

Jack and Virginia were much in love with each other, although they were very different. Jack was thin, had a great sense of humor, and loved company. He loved his liquor, especially after Virginia died of a brain tumor. He probably was not a very well read doctor, but his bedside manner was outstanding. I suspect