Sabine is a lunar crater that forms a nearly matching pair with Ritter to the northwest.
 The two rims are separated by a distance of only a couple of kilometers.
 To the west is the bowl-shaped crater Schmidt, to the northeast is the large ghost crater Lamont, and farther to the north are Manners (about 75 km) and Arago (about 125 km).
 Under a crater diameter to the south (25-30 km) is the equator.
 It is named after Edward Sabine.
Lawrence is a lunar crater that is located on a section of terrain to the east of Mare Tranquillitatis and northwest of Mare Fecunditatis and are named after Ernest and Robert Henry, Jr. Lawrence.
 To the southeast is the larger crater Taruntius.
 The rille designated Rima Cauchy crosses the eastern part of the Mare Tranquillitatis and reaches as far as the northern rim of Lawrence.
Bi Sheng is a lunar crater located on the lunar far side in the LAC-7 quadrant near the northern pole.
 The crater is located in close proximity to the prominent craters Seares, Karpinskiy, and Milankovic.
 The crater was adopted and named after Chinese inventor Bi Sheng by the IAU in August, 2010.
Secchi is a small lunar crater formation on the northwest edge of Mare Fecunditatis and is named after a 19th-century Italian astronomer Angelo Secchi.
 To the northeast is the crater Taruntius and nearly south is Lubbock.
 The western rim is joined with a section of the minor Montes Secchi range.
 The rim of this crater has been opened in the northern and southern ends, leaving two curved ridges facing each other across the crater floor.
 To the south is a pair of rilles designated the Rimae Secchi.
 These lie near the edge of the mare, and have a combined length of about 40 kilometers.
Harriot is a lunar crater that is located on the far side of the Moon from the Earth.
 It lies just to the north of the much larger crater Seyfert.
 To the northeast of Harriot is the crater Cantor.
 About one and a half crater diameters to the north of Harriot is the eastern end of a crater chain named Catena Sumner.
 This feature continues to the west-northwest for a distance of 247 km, passing to the north of the crater Sumner.
Breislak is a lunar crater that lies within one crater diameter north-northwest of the crater Baco, in the southern part of the Moon.
 To the north-northwest is the crater Barocius, and to the west lies Clairaut.
 This crater was named in honor of geologist Scipione Breislak.
Kaiser is a lunar crater.
 It lies in the crater-riddled terrain in the southern part of the Moon's near side, and is named after the Dutch astronomer Frederick Kaiser.
 The crater is nearly attached to the northeast rim the slightly larger crater Fernelius, and the two are separated by an irregular patch of ground only a few kilometers wide.
 To the northwest of Kaiser lies Nonius, a crater remnant.
Ernest Orlando Lawrence (August 8, 1901 – August 27, 1958) was a pioneering American nuclear scientist and winner of the Nobel Prize in Physics in 1939 for his invention of the cyclotron.
 He is known for his work on uranium-isotope separation for the Manhattan Project, as well as for founding the Lawrence Berkeley National Laboratory and the Lawrence Livermore National Laboratory.
Lipskiy is a lunar crater on the far side of the Moon.
 It lies just to the south of the lunar equator, and is the closest named crater to the antipode of the Earth zenith point.
 That is, it lies in the region of the Moon that is the most distant from the Earth.
 Lipskiy is located less than one crater diameter to the north of the prominent crater Daedalus.
 To the northeast is Krasovskiy.
Taruntius is a lunar crater on the northwestern edge of Mare Fecunditatis and is named after Lucius Taruntius Firmanus.
 To the northwest is the lava-flooded crater Lawrence, to the north lie the craters Watts and da Vinci and southwest is the crater Secchi.

Question: Of the two people that the Lawrence lunar crater is named after, which one was born August 8, 1901? 
Answer: Ernest Orlando Lawrence