Chushiro hayashi biography of rory
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Where is everybody? This common query represents the bewilderment of decades of futility in the search for extraterrestrial smart eller klok life (ETI). Part of the more recent disappointment stems from what scientists call the red sky paradox.1 It refers to at least five enigmatic facts.
The first fryst vatten that red dwarf stars are bygd far the most numerous stars in the universum, accounting for 78% of all nuclear-burning stars (stars that are actively fusing lighter elements into heavier elements) in the Sun’s vicinity.2 Second, red dwarf stars sustain nuclear burning much longer than other stars. Compared to the Sun, red dwarf stars maintain nuclear burning 20 times longer on average. Third, red dwarf stars, during their nuclear–burning history, brighten at a much slower pace than all other nuclear-burning stars. This slower brightening pace means more stable temperatures on the surfaces of planets orbiting red dwarf stars.
The fourth fact is that astronomers have observed a
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Ayako Wakao
ACTOR
1933 - Today
Ayako Wakao
Ayako Wakao (若尾 文子, Wakao Ayako, November 8, 1933 in Tokyo, Japan) is a Japanese actress who was one of the country's biggest stars of the 20th century. Read more on Wikipedia
Since 2007, the English Wikipedia page of Ayako Wakao has received more than 102,414 page views. Her biography is available in 15 different languages on Wikipedia. Ayako Wakao is the 3,924th most popular actor (down from 3,475th in 2019), the 1,158th most popular biography from Japan (down from 1,044th in 2019) and the 72nd most popular Japanese Actor.
Memorability Metrics
100k
Page Views (PV)
56.18
Historical Popularity Index (HPI)
15
Languages Editions (L)
1.83
Effective Languages (L*)
3.23
Coefficient of Variation (CV)
Among ACTORS
Among actors, Ayako Wakao ranks 3,924 out of 13,578. Before her are Ellen Schwiers, Ruby Dee, Ben Barnes, Andy Griffith, Kim Coates, and Debra Messing. After her are Rory McCann,
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Title: Growth model interpretation of planet size distribution
DOI: https://doi.org/10.1073/pnas.1812905116 ·OSTI ID:1509918
- Harvard Univ., Cambridge, MA (United States)
- Univ. of Texas, Austin, TX (United States)
- Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
- Georgia Inst. of Technology, Atlanta, GA (United States)
- Istituto Nazionale di Astrofisica–Osservatorio Astrofisico di Torino,