A Scenario for Interstellar Exploration and Its Financing by Giovanni F. Bignami, Andrea Sommariva

By Giovanni F. Bignami, Andrea Sommariva

This e-book develops a reputable state of affairs for interstellar exploration and colonization. In so doing, it examines:
• the current scenario and customers for interstellar exploration applied sciences;
• the place to head: the hunt for liveable planets;
• the motivations for area trip and colonization;
• the monetary mechanisms required to fund such businesses.

The ultimate portion of the ebook analyzes the uncertainties surrounding the offered state of affairs. the aim of establishing a situation is not just to pinpoint destiny occasions but additionally to spotlight the uncertainties which can propel the longer term in numerous instructions. Interstellar trip and colonization calls for a civilization during which humans see themselves as population of a unmarried planet and during which worldwide governance of those approaches is performed on a cooperative foundation. the foremost query is, then, no matter if our current civilization is prepared for such an exercise, reflecting the truth that the serious uncertainties are political and cultural in nature.

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Additional resources for A Scenario for Interstellar Exploration and Its Financing (SpringerBriefs in Space Development)

Example text

Then, this method would fail. Second, the method suffers from a high rate of false detections. Transit detection requires additional confirmation, typically from the radial-velocity method. However, when combined with the radial-velocity method, one can determine the density of the planet, learning something about the planet’s physical structure. One advantage of the transit method is that it makes possible to study the atmosphere of the transiting planet. When the planet transits the star, light from the star passes through the upper atmosphere of the planet.

If only the distance of one Cepheid from Earth could be found than it would be possible to anchor Leavitt’s measurement scale and estimate the distance for every Cepheid. This was accomplished few years later by Shapley and Herzsprung. The period-luminosity relationship for Cepheid made them the first “standard candle” in astronomy, allowing scientists to compute the distances to stars too remote for stellar parallax observations to be useful. It was now possible to measure the scale of the universe, which was done by Hubble who discovered that it was much bigger that astronomers imagined and that the Milky Way was just one galaxy among numerous others.

High probability of “life bearing” planets Closest system known to have one, and perhaps two or more planetary companions. Very small, low luminosity red dwarf (M5) Red dwarf star (M2) known to have a planet Single star system; slightly smaller and cooler than the Sun (K2), may have a planetary system similar to the solar system Large, hot white star (F5), second only to Altair in luminosity (within 20 light years). System contains small white dwarf Single star system, similar in size and luminosity to the Sun (G4).

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