Difference between revisions of "Timocharis"
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APOLLO OVER THE MOON; A VIEW FROM ORBIT, Chapter 5: Craters ([http://www.hq.nasa.gov/office/pao/History/SP-362/ch5.4.htm Part 4]), Figure 142 (Timocharis close-up).<br /> <br /> <br /> <br /> | APOLLO OVER THE MOON; A VIEW FROM ORBIT, Chapter 5: Craters ([http://www.hq.nasa.gov/office/pao/History/SP-362/ch5.4.htm Part 4]), Figure 142 (Timocharis close-up).<br /> <br /> <br /> <br /> | ||
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Revision as of 19:32, 11 April 2018
Contents
Timocharis
|
Lat: 26.7°N, Long: 13.1°W, Diam: 33 km, Depth: 3 km, [/R%C3%BCkl%2021 Rükl: 21], [/Stratigraphy Eratosthenian] |
Table of Contents
[#Timocharis Timocharis]
[#Timocharis-Images Images]
[#Timocharis-Maps Maps]
[#Timocharis-Description Description]
[#Timocharis-Description: Elger Description: Elger]
[#Timocharis-Description: Wikipedia Description: Wikipedia]
[#Timocharis-Additional Information Additional Information]
[#Timocharis-Nomenclature Nomenclature]
[#Timocharis-LPOD Articles LPOD Articles]
[#Timocharis-Bibliography Bibliography]
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images
- AS15-M-0600, 0599, 0598, and 0597 (four Mapping photographs of Timocharis, at the end of Revolution 22) are included in the book [/Light%2C%201999 Full Moon] by Michael Light and Andrew Chaikin (plates 37, 38, 39, and 40). Research: - DannyCaes DannyCaes Nov 27, 2007
Maps
([/LAC%20zone LAC zone] 40B3) LAC map Geologic map LTO map IAU Nomenclature Map (PDF)
Description
Description: Elger
([/IAU%20Directions IAU Directions]) TIMOCHARIS.--A fine ring-plain, 23 miles in diameter (the centre of a minor ray-system). It stands isolated on the [/Mare%20Imbrium Mare Imbrium] (below the level of which it is depressed some 3,000 feet), about midway between [/Archimedes Archimedes] and [/Lambert Lambert]. Its walls, rising about 7,000 feet above the floor, are conspicuously terraced, and on their E. outer slopes exhibit some remarkable depressions. There is a distinct break on the N., and a bright little crater on the N.E., connected with the foot of the glacis by a prominent ridge. On the bright central mountain, Schmidt, in 1842, detected a crater, which is easily seen under a moderately high light. Timocharis and the neighbourhood, especially the peculiar shape of the terminator on the W. of the formation, is well worth examination at sunrise.
Description: Wikipedia
Additional Information
- Depth data from [/Kurt%20Fisher%20crater%20depths Kurt Fisher database]
- Pike, 1976: 3 km
- Westfall, 2000: 3 km
- Viscardy, 1985: 3.11 km
- Cherrington, 1969: 2.86 km
- Timocharis C, D? and H are thermal anomaly craters, implying youthful ages - [/Moore%20et%20al%2C%201980 Moore et al, 1980]
- An elongated (and north-south oriented) depression at 24°30' North/ 18° West (east-southeast of Lambert and immediately west of craterlet Timocharis E) is mentioned in APOLLO OVER THE MOON: A VIEW FROM ORBIT, Chapter 7: Unusual Features (part 1), Figure 225. Note: this is an interesting target for lunar observers with powerful telescopes. Research: - DannyCaes DannyCaes Nov 27, 2007
- Included on [/ALPO%20list%20of%20bright%20ray%20craters ALPO list of bright ray craters]
- Included on [/ALPO%20list%20of%20banded%20craters ALPO list of banded craters]
- TSI = 30, CPI = 20, FI = 20; MI =70 [/Smith%20and%20Sanchez%2C%201973 Smith and Sanchez, 1973]
- David Barcroft (1897-1974) seems to have observed Timocharis "filled with vapor and very indistinct near Full Moon" (source: Epic Moon, page 309).
- V.A. Firsoff observed a red glow in Timocharis on the 8th and 10th of October 1954 (source: The Old Moon and the New, V.A. Firsoff, page 184), and a blue brightening on the 3rd of August 1955, as observed through a blue filter (page 185).
Nomenclature
- Named for Timocharis of Alexandria (ca. 320 BC - 260 BC), a Greek astronomer and philosopher. Likely born in Alexandria, he was a contemporary of Euclid. In approximately 3rd century BC, with the help of Aristillus, he created the first star catalogue in the Western world.
- An Internet search for a copy of that catalog leads to repeated statements that theirs (Timocharis and Aristillus') was the first, but no links to modern scholars who study Timocharis or his catalog or other works. His name is linked tightly to Hipparchos, however, because 169 years after Timocharis, Hipparchos compared his own star catalogue to Timocharis' and discovered that the longitude of the stars had changed by 2 degrees, which led him to determine the first value of the precession of the equinoxes.
- Timocharis B, the small bowl-shaped crater northeast of Timocharis, was called "Kovalevskij" on LTO-40B3 (prepared in April, 1974), for which it served as the title. Oddly, it is recorded as "a new name approved by the IAU", yet it appears not to have been approved. Kovalevskij is a variant spelling of [/Kovalevskaya Kovalevskaya], a name that had previously been approved (in 1970) by the [/IAU IAU] for an unrelated farside crater, and published in [/Menzel%2C%201971 Menzel, 1971]. How it came to be listed on the [/LTO LTO] as "approved" for the present nearside crater is unclear. It is included in Ewen Whitaker's list of [/Invalid%20Names Invalid Names].
LPOD Articles
Ringed with Almost Nothing Visible
Bibliography
APOLLO OVER THE MOON; A VIEW FROM ORBIT, Chapter 5: Craters (Part 4), Figure 142 (Timocharis close-up).
This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx4
