Thomas R CAVE

- Masatsugu MINAMI - (Director of the OAA Mars Section)

  from CMO #198 (25 December 1997)

  Tom CAVE, Jr

Tomas R CAVE   Tom CAVE is known as one of the most celebrated elders in the world of the Mars observation in the US: He started his career as a Mars observer from the 1935 opposition when he was just around 13 years of age, and thus the year before last in 1995 he welcomed his 60th anniversary of observing the red planet Mars. It was very natural that the ALPO congratulated him for his long life as a serious observer of Mars in July 1996 (see LtE in CMO # 182 p1961). In the oriental countries the number 60 has a special good implication because it is the least common multiple of 10 and 12.
Tom examines an ocular in 1948

  In addition to his life as a planetary observer, Tom CAVE has also been well known as a superb optician and maker having good gliding and polishing techniques and has long been an owner of Cave Optical Company from which he provided a great number of telescopes to the world.
  We should also recall that he has played an instructive role in amateur-astronomy world especially for the younger generations. For instance Samuel WHITBY recalls that, although they have never met in person, Sam has been aware of Tom's contributions since Sam's childhood, for Tom has published numerous articles that were instructive to the young Sam. (See Sam's LtE in this issue for more details.)
  It should again be noted that he is still an active observer of Mars who showed up several times in the present journal CMO even this year, and it is our pleasure to pay homage to Tom CAVE on this occasion here by learning back his younger days.

15cm f/10 Reflector

  We hear it was 8 years old in 1930 when he was first attracted by Astronomy by visiting the Adler Planetarium in Chicago several times. He was at that date deeply influenced by an uncle in-law who was an MIT Master of Science.
  His family moved to Los Angeles in 1931 and then to Long Beach in the early spring of 1934 where he began to practise the dark skies and telescopes. He also read some books on astronomy for pre-teenagers. He began to learn the constellations by naked eyes plus a pair of binoculars used in WWI. In summer vacation time when he was in the sixth grade of elementary school in 1934, he earned some money by mowing neighbour's lawns to buy an achromatic 6.3cm refractor-tube assembly which was equipped with a 20mm eyepiece. He remembers clearly the day it reached him at the beginning of the 1934 autumn. Here his father, Tom CAVE Sr, made an appearance to provide his son with a set of tripod having an equatorial mounting. The skies at Long Beach was dark enough to watch several stellar objects.
  Meanwhile Tom Jr came to know the existence of the Long Beach Telescope Makers Club on a newspaper, and this became very decisive to him in several senses. First he was led to have a free kit of a 15cmx2.5cm thick plate glass from which he tried to make an f/10 mirror. This was really well polished and figured since he was helped by several professional opticians. The tube which accommodated the speculum needed a 150cm length as well as the Mt Wilson's 250cm type mounting. This was again helped by CAVE Sr. This telescope was completed by the 1934 Christmas, and already his parents had given him three Ramsden eyepieces by J E MELLISH which gave him magnifications 90x, 180x, and 310x.
  Those days, the Telescope and Astronomy Clubs at the district were very active, and several f/6 and f/7 Newtonians were possessed by the members. However CAVE Jr, upon visiting and trying to watch the lunar and planetary objects by use of these shorter telescopes, was somewhat disappointed at the performances and became convinced that f/9 - f/11 Newtonians could give much clearer and sharper images of the planets. Note that this conviction occurred to a boy at the age of 12. The boy was thus, as it were, father to the latter Tom CAVE.
  In 1935, he watched the Messier objects, clusters, double stars as well as planets by using both telescopes. Especially he began to view the planet Mars by the 15cm f/10 reflector and made some rough drawings of the markings. Mars was at opposition in April. Tom detected Syrtis Major and Mare Acidalium. He also read some books which he obtained at the second-hand bookstore: For example he bought P LOWELL's first book on Mars published in 1895 at a cost of 2 dollars.

Apparitions of Mars in 1937 and 1939

  In 1937 Mars was closest to the Earth in May. This was the apparition when Tom began his systematic series of the Mars observations by use of the 15cm f/10 reflector, and he made a few dozen drawings during the season. The best dozen were sent to Harold B WEBB at Long Island, NY and they were published later. The 1937 apparition was therefore the first fruitful one for Tom, just 60 years ago and the same time when Tsuneo SAHEKI here in Japan observed the planet at the Kwasan Observatory (see CMO #175 p1840). The same year Tom read through W H PICKERING's Mars Reports at the Long Beach Central Library.
  In 1938 summer, Tom went to Chicago and at the basement of the Adler Planetarium he met Edwin P MARTZ Jr who in turn told him of the addresses of some lunar and planetary observers including Walter H HAAS, Hugh M JOHNSON and Frank VAUGHN. In 1939 Tom began to correspond with these observers, and exchanged the observations. In 1939, Tom observed intensively the planet Mars which approached perihelically the Earth in July (the maximal apparent diameter was 24.1 arcsecs). He obtained a considerable number of drawings. He learned also how to use the American Ephemeris.
  The Los Angeles Times then carried an article on Mars written by a professional astronomer at Mt Wilson Observatory, and Tom wrote a letter to the Observatory and immediately received a reply from Dr Robert RICHARDSON who invited Tom to Mt Wilson to observe Mars by use of a 150cm reflector. On the appointed evening, a relative of Tom's drove him up; the seeing was very good that night and the view of Mars was very excellent: Since then until his death, Dr RICHARDSON was a close astronomical and social friend of Tom's.

25cm f/11.2 Reflector and the 1941 Apparition

  In early spring of 1940, his family purchased a home in a best residential part of Long Beach, and Tom and his father built a 4.2mx4.2m square observatory having a dome imitating Mars Hill's one. He made a 25cm Pyrex mirror having 280cm focal length in a square plywood tube mounted on the German form of equatorial mount.
CAVE's Mars-Hills-type Observatoy at Long Beach in 1940

  In 1941 Mars was at opposition in October and the year was very fruitful to Tom: In January 1941 he finished high school, and at once secured employment through the Los Angeles Astronomical Society at Herron Optical Company (for 60 hrs a week). At night he was rather free at home and was able to observe Mars from May to December and obtained a total of 254 numbers of drawings. This is still his record number for one season. Most drawings were made using loaned Zeiss & Leitz orthoscopic and monocentric oculars (far better than Ramsden).
In October Tom detected a marking which was new to him near at LCM=200° W , and so sent the drawing to Dr E C SLIPHER at Lowell. Within days, a reply came from E C SLIPHER himself who identified the marking to be the detached Lastrygonum Sinus. SLIPHER asked Tom to send more sketches and in November he invited Tom to join the Lowell staff as an observing assistant of the planets. It was a honour to Tom, but since he was working as an apprentice optician at Herron Optical Co, he felt he had to turn down the offer.

  After the US entered WWII, the Herron Optical employees zoomed up from 21 to 155, while Tom himself was enlisted in the US Army: He was sent in the European theatre, and a few days after the liberation of Paris on 25 August 1944, he had a chance to visit the Meudon Observatory which was his only astronomical experience he had in Europe during the war time.
From Tom's drawing in 1941 (340x 25cm spec)
16 Oct 1941 (Ls=292°, LCM=252°W, De=21°S)

  Returning home at the beginning of 1946, Tom entered the University of Southern California (which was located only a few block walk from Herron Optical Co) and at the same time he went back to work at the Company 40 hrs a week doing optical work on motion pictures. With study and work, in the 1946 apparition (opposition in January 1946) he could not obtain more than ten or twelve drawings of Mars.

At Lowell Observatory in 1948

  Prior to the 1948 aphelic apparition (opposition in February), Tom made a 20cm f/10 reflector which was mounted on a Thomas Cooke & Sons clockdriven equatorial mount.
  In the 1948 Easter break Tom attended the meeting at Lowell and met for the first time E C SLIPHER, V M SLIPHER and C O LAMPLAND. E C SLIPHER allowed Tom to observe the planet for several nights by use of the Clark 60cm Refractor: Tom on the occasion much learned about the planetary visual observations. He thus made observations of Mars at Lowell as well as by use of the 20cm Reflector.

31cm Monster Telescope

The monster 31cm f/11.3 Newtonian built in 1950: Tom at age of 27
  In 1949 he ground and polished a 31cm speculum having a 335cm focal length. This was accommodated in a long rotating tube of 3.6m (12 feet) in length which was electrically clockdriven. This telescope was probably the best ever Tom made, and gave good performances under good seeing allowing 400x, 800x. He used this monster in the 1950 and 1952 apparitions. O R NORTON, who once worked under Tom CAVE, wrote later (S&T vol 88 August 1994 issue p88) about his first experience meeting with this telescope as follows: " I arrived at 265 Roswell Av and passed through the gate to the backyard --- and into another world. Before me stood a leviathan of a telescope, so large that it would have taken a 12-foot ladder to reach the eyepiece."

Cave Optical Company

  Still attending the USC, he polished a lot of 15cm, 20cm, 25cm and 31cm specula for amateurs in Los Angeles and before December 1950 he had made more than 900 mirrors. CAVE Sr so decided that Tom should run his own optical business in a 9mx26m store a mile apart from their home. CAVE Sr built several modified Draper polishing machines and et al. In mid-December 1950, CAVE Sr and Jr entered full time business: They received a large order for the primary mirrors, and then for tube assemblies and the mounting systems, and by late 1951 they were to do the telescope business; this becoming eventually Cave Opitical Company. This Company continued until 1980, and for the last ten years they had 30 - 35 employees and 8 persons who figured mirrors and objective lenses.
  NORTON also belonged to the Company and tells us an episode about CAVE Sr who was a wonderful man: " One day in the middle of one of these (coffee) breaks, the secretary called Cave to the front office. Although Cave was never harsh or demanding, he returned from there red faced and obviously upset, numbing something unrepeatable about his father. Cave Sr ran the business affairs of Cape Optical and was essential to its early success. He also had wonderful handwriting. With a diamond pencil he scribed the Cave Optical signature on the back of each mirror, complete with focal length and mirror number. Each mirror was fine ground flat on the back, clearly distinguishing it from the front. But on that day the elder Cave had blundered: a just-completed 6-inch mirror on his desk bore the beautiful Cave Optical inscription ---on the front! We never let him forget that day." NORTON also writes " I regret that I did not have him scribe a mirror for me in his Old English style. A thousand mirrors bear his distinctive mark, and lucky is the amateur who has one." The present writer wonders if Alan HEATH's Cave mirror has the Old English signature or not.
  CAVE Sr passed away in 1957, and since then CAVE Jr became Thomas CAVE.

International Mars Committee and IMP

  In 1953 Tom was invited in Colorado to join the International Mars Committee. In 1954, 1955, and 1956 it was held at Lowell. Tom attended all of these meetings. (The Japanese Committee of the IMC was then held asked by E C SLIPHER and organised by I YAMAMOTO, President of the OAA.) The outgrowth must have been the International Mars Patrol in America. The late Charles (Chick) CAPEN and Tom observed Mars three apparitions in the 1960's from the JPL Table Mountain Observatory. The CAPENs had a nice cabin as well as a guest cabin; Tom's late wife and two teenaged daughters stayed many weekends when Tom was observing with CAPEN using 40cm and 60cm telescopes. The seeing at the Table Mountain was often excellent.
  Tom played a role of Assistant Recorder of the ALPO Mars Section from April 1969 to January 1974 when CAPEN was the Recorder.
27 Mar 1950 ( 400x 20cm Newtonian )
Ls=096°, LCM=091°W, AppDia.=14.4"

  Tom also visited several times E C SLIPHER when he was in the residence at Lowell. The Mars Committee Conferences had many notable professional astronomers one of whom Tom met was Andrew E DOUGLASS (1867 - 1962). Note that DOUGLASS lived nearly one century: He observed Mars in 1892 with W H PICKERING in Peru with a 33cm Refractor and two years later at Flagstaff as a staff of P LOWELL. He often used a 20cm Clark Refractor and a 90cm Stewart Reflector stopped down to 33cm for Mars observations.

Great Apparition in 1956

27 Mar 1965 ( 500x 33cm Newtonian )
Ls=088°, LCM=247°W, AppDia.=12.5"

  In 1956 and again in 1971, Tom was invited by Robert RICHARDSON to observe the red planet with him at Mt Wilson by use of the 150cm and 250cm telescopes, both using the Coude focus. On 10 August 1956 (the App Dia =21.8", 240° Ls), they had a perfect seeing for longer than 30 minutes on the 250cm Coude and observed visually with 1000x, 2500x, and even over 3000x. This must have been quite the same experience as E M ANTONIADI had on 20 September 1909 at the eyepiece of the 83cm refractor when the sky over Meudon was very calm for half an hour, but Tom and RICHARDSON believed that they had a far better visual look on the 250cm, and thus they forgot to take pictures. Tom writes: "The planet had extremely fine details and we felt that we were flying over the planet. The view was the most amazing one of Mars perhaps anyone has ever had from land-based stations. The steady view was totally beyond human description. There were no canals, just only exceeding fine broken details . . . . Mts of Mitchell detached from the spc. At no other time have I seen more than 10% or 15 % that we saw that night."
  As he remembers, another occasion of near perfect seeing occurred to him in October 1941 at his Observatory using 25cm f/11 when he saw clearly Iuventa Fons as a tiny black drop of ink with a perfect diffraction ring around it.

From left to right:
12 June 1971 (Ls=196°, LCM=353°W);
13 June 1971 (Ls=197°, LCM=332°W);
16 June 1971 (Ls=198°, LCM=312°W)
Three from 197 drawings made in 1971 much before opposition around when AppDia.=16" by use of 500x 31cm spec

Recent Years

  Anyway as to the telescopes amateur planetary observers use, Tom has believed in the system of Newtonian, and produced and provided a great numbers of Newtonians having good specula to the world of thousands of amateur astronomers. However this showed a slight retrospective aspect because recent years the shorter Schmidt- Cassegrains or otherwise more rough Dobsonians have become popular. This fact brought some difficulties to the business of Cave Optical Co at the end of the 1970's.
  Furthermore in the spring of 1979, Tom seriously suffered from kidney illness and nearly died, as he describes. Hospitalised for many weeks and receiving a massive operation and needed a rehabilitation at home, he was at last forced to sell the business which he maintained for more than 30 years: During the time, Cave Optical Co produced 83,000 prime-mirrors including refiguring of the amateur-made mirrors and a large number of mirrors made for NASA, the largest having a 75cm diameter. Telescopes including the optical tubes and equatorial mounts are totalled over 16,000.
  Tom then ran an optical shop for Hughes Aircraft Co and worked briefly for Perkin Elmer, but retired in 1988.
  Tom has remained however to be a Mars observer, and he has long been our member of the CMO.
  We have missed to mention the telescopes he is using at present. We expect he himself will mention the story of these telescopes in the future. (Or see the S&T photo-illustrations in NORTON's article.) The main must be a 32cm Newtonian with a shorter focal length to be housed in the old square Observatory. It is piggybacked by a 14cm Clark Refractor of which he looks to be proud. We should note that by the use of the 32cm spec he contributed to us this 1996/97 apparition a total of 33 drawings of the red planet. After all, he has been watching Mars about over 3000 times since 1935, and we sincerely hope he will continue at least up until the upcoming great apparition in 2003.


  We are very thankful to Tom for his kind information and labour, and furthermore for giving us his precious photos and drawings to be produced here.
  We are also indebted to Sam WHITBY who has encouraged us to write about Tom, kindly phoned Long Beach up and communicated several informative points to us.

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