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The Moon Shot
The First Seven Astronauts
Everything starts somewhere, and the space program began in earnest with the selection of the first seven astronauts that would participate in manned space flight. The NASA selection committee was made up of Charles Donlan, a senior management engineer; Warren North, a test pilot engineer; Stanley White and William Argerson, flight surgeons; Allen Gamble and Robert Voas, psychologists; and George Ruff and Edwin Levy, psychiatrists.
When the selection committee began their task, they received 508 applications. This number was reduced to 110 candidates after records were reviewed. The 110 candidates were brought together at an undisclosed location. A battery of tests were given and interviews were conducted. It took a month but the number of possible candidates was reduced to 32.
The 32 candidates were then subjected to even more stressful physical, psychological, and mental examinations. They were given full-body x-rays, tested in pressure suits, endured a variety of cognitive tests and really intense interviews. Finally, 18 or the 32 were recommended to the Mercury program without any medical reservations.
The final choices were made by Robert Gilruth, who was the head of the Space Task Group, as well as Charles Donlan, Warren North, and Stanley White.
The first seven astronauts selected for the Mercury program (the first manned space flight program) were Scott Carpenter, L. Gordon Cooper Jr., John H. Glenn Jr., Virgil I. "Gus" Grissom, Walter M. Schirra Jr., Alan B. Shepard Jr., and Donald K. "Deke" Slayton. Their names will resound through history forever.
Six of the original seven flew in Project Mercury. Only "Deke" Slayton did not fly because of a heart condition that had not been discovered. Deke later flew as a crewmember of the Apollo-Soyuz Test Project.
See Also:
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Nicolaus Copernicus
The Stars
Our sun is a star. It is one of the billions of stars in the Milky Way Galaxy. On a clear night, when you look up at the sky, you can see thousands of stars with your naked eye. If you have a pair of binoculars or a telescope, you can see more stars than you could ever hope to count.
Each star is unique, but they all share things in common as well. Stars are born from interstellar gas clouds, nuclear fusion causes them to shine and stars die. Sometimes the death of a star is a very dramatic event.
Cold interstellar clouds or nebula, like the Orion Nebula and the Eagle Nebula, are the incubators and nurseries from which stars are born. An extremely simplified description is that gravitational collapse happens and forms a rotating gas globule. The resulting globule spins faster and faster. The central core becomes a star while the other material becomes planets or asteroids.
The life of a star begins and ends with a battle between two forces: gravity and pressure. It takes energy for a star to live, and this energy comes almost entirely from nuclear fusion of lighter elements into heavier elements. This is the energy through which a star can shine for millions or billions of years.
Stars fuse hydrogen to helium for most of their lifetime. This is referred to as the "main sequence" of a star's life. Our sun, Vega, Sirius, and Spica are all stars that are in their main sequence. Once the hydrogen in the core of a star has been used up, the star becomes a red giant like Betelguese, Arcturus, Aldebaran and Antares.
A star's life is limited because the hydrogen at the core is not self-replenishing and will eventually be used up. A star cannot depend upon thermal energy to resist the pull of gravity forever, and a star's final fate depends on whether something other than thermal pressure manages to halt the relentless crush of gravity. |
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Inspired by Maria Mitchell
Generations of women scientists in all of the scientific disciplines have been inspired by Maria Mitchell. Ms. Mitchell was a woman ahead of her time who left an indelible mark on science and the role that women play in scientific research and discovery.
Maria Mitchell was born in 1818. A Quaker couple, William and Lydia Mitchell, had 10 children; Maria was the third child. She attended Cyrus Peirce's School for Young Ladies in her early years, then was taught mostly by her father. After that she was mostly self-educated, but she was the first woman to ever have an advanced degree awarded. It was awarded by Indiana Hanover College in 1853 after she had already discovered a comet, which is named after her. She was also the first woman ever appointed to the Academy of Arts and Sciences.
Maria Mitchell was the most famous American scientist of either sex in the nineteenth century. She was a most remarkable woman who left her mark on astronomy long before women gained the right to vote. In 1847, Maria discovered what we know today as the Comet Mitchell 1847VI, and that was just the first in a long list of accomplishments.
Maria Mitchell is still inspiring young astronomers today. The Maria Mitchell Observatory was established next to her home in Nantucket, Massachusetts, in 1908, and it is still very much operational. There is an extensive public education program, and the observatory sponsors research by undergraduate students. The Maria Mitchell Observatory is funded by the National Science Foundation.
The Maria Mitchell Observatory is also home to over 8,000 historic photographic glass plates. The plates were taken by observatory astronomers and students between 1910 and 1995 and span nearly a century of the Nantucket night skies.
Related Topics: The Planet Neptune,
Asteroids, Comets and Meteors, Our Sun's Twin
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