
American physicist (1868–1953)
Missing: 4, 5, 7, 9. Present digits repeat to show how many times they occur.
Three is the number of expression — the point at which a thing becomes shareable. Tradition links it to language, humour, performance and the ability to make an idea land. It is generally read as the most immediately likeable number, and the reading usually adds a warning in the same breath: fluency can outrun substance, and 3 is described as capable of talking its way past work it has not actually done.
A complete line in the grid.
A complete line in the grid.
A complete line in the grid.
Concentrated expression. Read as a voice that arrives before the edit does.
Read as impatience with structure and maintenance. Associated with starting well and leaving the scaffolding to someone else.
The centre of the grid, so its absence is weighted heavily. Read as difficulty adapting mid-course — a preference for the plan already chosen over the plan now indicated.
Read as reluctance to sit with an unresolved question. Associated with wanting the working answer rather than the true one.
Read as a narrowed field of view: strong loyalty close in, less pull from causes further out.
Moolank 4 comes from the day of the month alone; Bhagyank 3 from the whole date. They differ, which is the ordinary case — the two numbers answer different questions.
The ascending lunar node — a shadow graha, not a physical body. Disruption, ambition, the unconventional. Read with more caution than any other.
Bhagyank uses the same arithmetic as the Western life path, so the two will always agree. That is not two traditions confirming each other — it is one calculation under two names.
Science walks forward on two feet, namely theory and experiment.
Since the origin of the "penetrating rays" was still uncertain, Dr. Russell Otis and myself in the summer of 1923 went to the top of Pike's Peak for the sake of making absorption experiments upon these radiation at the highest altitude to which we could carry large quantities of absorbing materials. For if the rays were not of cosmic origin they did not need to be more penetrating than are the gamma rays from radioactive materials, while if they were of cosmic origin the sounding balloon experiments of Bowen and myself had shown that they must be very much harder (more penetrating) than anybody had thus far assumed. What was needed was absorption experiments to determine just what sort of rays they actually were.
In 1832 the English astronomer Airy, in making a report to the British Association on the state of astronomical science throughout the world, remarked that he was unable to say anything about America astronomy because, so far as he knew, no public observatory existed in the United States. It was in the 1840's that the Cincinnati Observatory, the Naval Observatory in Washington, and the Harvard College Observatory in Cambridge, Massachusetts, were founded—the three pioneer institutions in a development that has continued with increasing acceleration ever since.
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