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Endangered Species - The Hawksbill Turtle

The hawksbill turtle's status has not changed since it was listed as endangered in 1970. It is a solitary nester, and thus, population trends or estimates are difficult to determine. The hawksbill is a small to medium-sized sea turtle. The following characteristics distinguish the hawksbill from other sea turtles: two pairs of prefrontal scales; ...

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EndangeredSpeciesHawksbillTurtle
Geology

1816 - The Year Without A Summer

Most global temperature change occurs over a long period of time, centuries rather than years, and in small increments. But in 1816, the Northeastern part of the United State and Northern Europe were ... Continue reading

1816YearSummer
Biology

Microorganisms: Are they really that bad?

We buy antibacterial hand soaps and cleaners to get rid of microorganisms that we don't want around us or our homes, but can some of them actually be helpful? You may think that they only cause harm, ... Continue reading

Microorganisms
Physics

What Is Radiofrequency Energy (Rf)?

Radiofrequency (RF) energy is another name for radio waves. It is one form of electromagnetic energy that makes up the electromagnetic spectrum. Some of the other forms of energy in the ... Continue reading

WhatIsRadiofrequencyEnergy
Biology

New Ideas About An Old Puzzle

There's a familiar way of talking about language as a 'tool,' but of course that's just a metaphor. Literal tools made of rock can last for millennia as evidence of the skills of early humans. Not so ... Continue reading

NewIdeasAboutAnOldPuzzle

Subrahmanyan Chandrasekhar

SubrahmanyanChandrasekharNASA's premier X-ray observatory was named the Chandra X-ray Observatory in honor of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar (pronounced: su/bra/mon'/yon chandra/say/kar). Known to the world as Chandra (which means 'moon' or 'luminous' in Sanskrit), he was widely regarded as one of the foremost astrophysicists of the twentieth century. Chandra immigrated in 1937 from India to the United States, where he joined the faculty of the University of Chicago, a position he remained at until his death. He and his wife became American citizens in 1953.

Trained as a physicist at Presidency College, in Madras, India and at the University of Cambridge, in England, he was one of the first scientists to combine the disciplines of physics and astronomy. Early in his career he demonstrated that there is an upper limit - now called the Chandrasekhar limit - to the mass of a white dwarf star. A white dwarf is the last stage in the evolution of a star such as the Sun. When the nuclear energy source in the center of a star such as the Sun is exhausted, it collapses to form a white dwarf. This discovery is basic to much of modern astrophysics, since it shows that stars much more massive than the Sun must either explode or form black holes.

Chandra was a popular teacher who guided over fifty students to their Ph.D.s. His research explored nearly all branches of theoretical astrophysics and he published ten books, each covering a different topic, including one on the relationship between art and science. For 19 years, he served as editor of the Astrophysical Journal and turned it into a world-class publication. In 1983, Chandra was awarded the Nobel prize for his theoretical studies of the physical processes important to the structure and evolution of stars. According to Nobel laureate Hans Bethe, 'Chandra was a first-rate astrophysicist and a beautiful and warm human being. I am happy to have known him.' 'Chandra probably thought longer and deeper about our universe than anyone since Einstein,' said Martin Rees, Great Britain's Astronomer Royal.