Needed: tenable values or five to ten more earth-sized planets. Interview by Desmond Avery.

نویسنده

  • J Last
چکیده

John Last has worked as a ship’s surgeon on intercontinental voyages, an epidemiologist and university teacher in Australia, Canada, the United States and the United Kingdom, and a consultant in numerous developing countries. He has won prestigious awards for his contributions to epidemiology and preventive medicine. Among his current preoccupations is the blindness of the media, the general public and decision-makers as to what is really at stake globally for human health now and in the coming years.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

An Earth-sized planet in the habitable zone of a cool star.

The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 ± 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-size...

متن کامل

Observed properties of extrasolar planets.

Observational surveys for extrasolar planets probe the diverse outcomes of planet formation and evolution. These surveys measure the frequency of planets with different masses, sizes, orbital characteristics, and host star properties. Small planets between the sizes of Earth and Neptune substantially outnumber Jupiter-sized planets. The survey measurements support the core accretion model, in w...

متن کامل

1 FRESIP : A Mission to Determine the Character and Frequency of Extra - Solar Planets Around Solar - like Stars

FRESIP (FRequency of Earth-Sized Inner Planets) is a mission designed to detect and characterize Earth-size planets around solar-like stars. The sizes of the planets are determined from the decrease in light from a star that occurs during planetary transits and the orbital period is determined from the repeatability of the transits. Measurements of these parameters can be compared to theories t...

متن کامل

Terrestrial Exoplanet Light Curves

The phase or orbital light curves of extrasolar terrestrial planets in reflected or emitted light will contain information about their atmospheres and surfaces complementary to data obtained by other techniques such as spectrosopy. We show calculated light curves at optical and thermal infrared wavelengths for a variety of Earth-like and Earth-unlike planets. We also show that large satellites ...

متن کامل

Superhydrophobic surfaces reduce drag

Rare and common The hot grains of tektite and obsidian that show up in HD 172555’s IR spectrum are small enough that the star’s radiation pressure would drive them away from their current 6-AU orbit within 0.1 million years. The SiO molecules would likely condense and reform minerals on the same time scale. Given that rocky planets take 100 My to form, catching a giant impact in HD172555, despi...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:
  • Bulletin of the World Health Organization

دوره 79 9  شماره 

صفحات  -

تاریخ انتشار 2001