The Constitution of the Republic of Hawaii

This chapter traces Kurihara's childhood in Hawaiʻi. Kurihara was born on January 1, 1895, two years after the overthrow of the Hawaiian monarchy and three years before the U.S. Congress passed a joint resolution that resulted in the occupation of the islands as an American territory. Kurihara first attended Kaiulani School in September 1903. Like his classmates, many of whom were also children of immigrants, Kurihara was a U.S. citizen because he was born in Hawaiʻi. According to the Organic Act, which created the Territory of Hawaii, all who had been citizens of the Republic of Hawaii—which meant those born or naturalized in the Hawaiian islands—were “declared to be citizens of the United States.” In race-conscious America in the early twentieth century, however, the meaning of citizenship for racial and ethnic minorities was amorphous. Thus, Kurihara and other Asian Americans were often treated as noncitizens or as “new” Americans.

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The Establishment of the Republic of Hawaii, 1893-1894

Pacific Historical Review ◽

10.2307/3633128 ◽

1935 ◽

Vol 4 (3) ◽

pp. 201-220 ◽

Cited By ~ 10

Author(s):

Donald Rowland

Keyword(s):

The Republic ◽

Republic Of Hawaii

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Time and Latitude in South Africa

International Astronomical Union Colloquium ◽

10.1017/s0252921100026816 ◽

1972 ◽

Vol 1 ◽

pp. 27-38

Author(s):

J. Hers

Keyword(s):

South Africa ◽

Cape Town ◽

Astronomical Observations ◽

Royal Observatory ◽

The Republic ◽

Astronomical Determination ◽

Limited Accuracy ◽

Better Than

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.

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