A
century later, Hipparchus wrote of a
total solar eclipse at Hellespont that was
4/5th eclipsed at Alexandria. He used
this to calculate that the lunar distance
was between 62 and 72 + 2/3 earth
radii. He was careful to use ranges
rather than precise distances. He calculated the solar distance as greater
than 490 earth radii. | Object | Ptolemy / Sun | Ptolemy's angle | Today's angle | Today's Brightness |
| Sun | 1/1 ratio | 31' 20" | ~32' 42" | -26.7 |
| Mercury | 1/15th of Sun | 2' | 13" | -1.9 |
| Venus | 1/10th of Sun | 3' | 1.1' | -4.6 |
| Mars | 1/20 of Sun | 2' |
|
-2.91 |
| Jupiter | 1/12 of Sun | 2.6' |
|
-2.94 |
Astronomers
can determine the Sun's distance by measuring the Martian parallax. In
October
1672
Mars occulted Psi Aquarius while at opposition. Giovanni Cassini sent
Jean Richer to
South America to measure the background stars during the
occultation. Cassini measured the same stars from Paris. Their
simultaneous parallax was 25" of arc. On October 6, 1672, John
Flamsteed used a micrometer eyepiece to measure the diurnal
parallax at just under 25". Mars was at a turnaround point
so it
was almost stationary relative to earth. Flamsteed calculated the
maximum solar parallax as 10" or 81.7 millions miles. Cassini
calculated 9.5" for a solar distance of 86 million miles. Their
parallax measurements resulted in a solar distance 6 to 7%
smaller than today's accepted value. Astronomers continued to
measure the solar parallax during the next three centuries. | Astronomer | Parallax Date | Type | Solar Parallax | AU million miles |
| Flamsteed |
|
Mars Diurnal |
10" - |
81.7 |
| Cassini |
|
Mars Occultation | 9.5" | 86 |
| LaLonde |
|
Venus Transit | 8.85 to 8.63" | 94.7 |
| Pingre |
|
Venus Transit | 8.80" | 92.885 |
| Enke |
|
Transits Venus | 8.55776" | 95.250 |
| Hall |
|
Mars Meridian | 8.842" | |
| Todd |
|
Venus Transit | 8.883" | |
| Obrecht |
|
Venus Transit | 8.881 | |
| Proctor |
|
Venus Transit | 8.880" | 92.558 |
| Harkness |
|
Venus Transit | 8.809" | 92.797 |
| Newcomb | 1892 | Aberration Sunlight | 8.79 - 8.80' | using clocks |
| Jones | 1941 | Eros opposition | 8.79" | |
|
|
Radar | 8.794148" | 92.955859 | |
| Many astronomers |
|
41 parallax measurements Venus transit | mean of parallax measurements 8.538" | 95.740 |

Here is a tiny portion
of the Hubble
Ultra Deep Field. Galaxy #3180, lower left corner, has two arms of
equally
spaced star clusters. Its light shines at
half the frequencies of local atoms. In
the upper right, #3031 has two arms
made of equally spaced clumps that
have rotated around less than one
turn. The light from this galaxy clocks
four tenths the frequencies of similar
local atoms. The light from the long
chain galaxy, #3178 left center, clocks 90% of the light frequencies of
local atoms. The short
blue chain galaxy, #3306 - top center, has four equally spaced beads -
like a necklace. Its light
clocks six tenths the frequencies of similar local atoms.