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Dust in Space - Max-Planck
Dust in Space - Max-Planck

... there are large numbers of meteorites on Earth. These are fragments of asteroids that have left their original orbit, which is mainly between Mars and Jupiter, and collided with the Earth. There has been comet dust in terrestrial laboratories for years. Comet particles enter the upper atmosphere, wh ...
where do space rocks come from?
where do space rocks come from?

... Meteorites, asteroids, comets – they’re all kinds of space rocks aren’t they? The terminology can be confusing and often is confused – by journalists and scientists as well! Use this lesson to chat about what the different terms mean and ways to remember them, and to pique the curiosity of your stud ...
Giant planet formation
Giant planet formation

... Gravitational instabilities in the protoplanetary disk form clumps of material, the protoplanets, with the solid parts settling in their cores. “Top-down planet formation” Main advantages of the disk-instability hypothesis: • It explains the similarities between stars, brown dwarfs, and gas giants • ...
INTERSTELLAR FLIGHT: ASPECTS OF BEAMED ELECTRIC 88
INTERSTELLAR FLIGHT: ASPECTS OF BEAMED ELECTRIC 88

... published performance projections for electric rockets. A representative one-way centuries-long interstellar exploration/colonization mission is defined in terms of mass alloments. For this mission, a comparison of beamedelectricramjetand rocketperformanceispresented. It is shown that rockets and ra ...
Formation and Detectability of Terrestrial Planets around
Formation and Detectability of Terrestrial Planets around

... endowed with circumprimary disks containing a relatively high fraction of solid material. Simulations such as the ones we have performed and others indicate that the final mass present in terrestrial planets is in direct proportion to the initial amount of material available. α Cen B is exceptionall ...
From planetesimals to planetary systems: a hardles race
From planetesimals to planetary systems: a hardles race

... Dust coagulation model PROs: Smooth grow of larger bodies  Reliable collisional model  Initial size distribution of any kind  Robust (it does not depend much on initial parameters)  It can overcome the 1-m catastrophe ...
A Planetary System Around Our Nearest Star is Emerging
A Planetary System Around Our Nearest Star is Emerging

... Centauri B, is almost as large as Pluto as seem from Earth. Unfortunately, astronomers do not have the capability and detect the light from Alpha Centauri Bb from the star. Exoplanets are detected because they affect their pare ...
Temperate Earth-sized planets transiting a nearby ultracool
Temperate Earth-sized planets transiting a nearby ultracool

... age constrained to be more than 500 million years (Myr), and with a luminosity, mass and radius of 0.05%, 8% and 11.5% those of the Sun13, respectively. We determined its metallicity to be solar through the analysis of newly acquired infrared spectra. The small size of the host star—only slightly la ...
Sample Schedule 2012
Sample Schedule 2012

...  have solid surfaces and thin or no atmospheres  have varied atmospheres ranging from no atmosphere (Mercury) to a thin atmosphere consisting mainly of nitrogen and oxygen (Earth)  spin slowly compared to the outer planets  have no or few moons (Earth has 1 moon, Mars – 2)  have no rings orbiti ...
The Prospective Aspect of the Cosmogonic Models in Laozi and T
The Prospective Aspect of the Cosmogonic Models in Laozi and T

... momentum being less than of its surrounding planets and of the sun originating before the planets. – It was harshly attacked by Safronov, who felt that time needed for a thin cloud envelope to develop into planets would exceed the age of the solar system. ...
Lecture 13 - Star Formation
Lecture 13 - Star Formation

... monoxide map ...
Introduction
Introduction

... been detected using the same technique, based on the precise radial velocity measurements of the host star. In this Section, we briefly review this and other techniques used to detect exoplanets, paying special attention to their major findings and the current status. After that (Section 1.2), we wi ...
CVs
CVs

... – Usually this would cause the star to slow down its ...
The most common habitable planets – atmospheric characterization
The most common habitable planets – atmospheric characterization

... As for the contribution of the solid surface of the planet to the thermal balance, the low thermal inertia of the various possible materials (Putzig & Mellon 2007) does not measure up with the thermal capacity of a substantial atmosphere. In the case of Mars, for example, there is around 174 kg of a ...
4. The Solar System
4. The Solar System

... • The star Beta Pictoris is surrounded by a disk of warm matter, which may indicate planetary formation. ...
A Comment on “The Far Future of Exoplanet Direct Characterization
A Comment on “The Far Future of Exoplanet Direct Characterization

... Nevertheless, even if future work does reveal the presence of a significant population of large interstellar grains in the LIC, it is, contrary to the impression given by Schneider et al. (2010), certainly possible to envisage appropriate countermeasures. Schneider et al. stated that “no currently ...
latest Edition - ExoPlanet News
latest Edition - ExoPlanet News

... Kepler-78b is one of a growing sample of planets similar, in composition and size, to the Earth. It was first detected with NASA’s Kepler spacecraft and then characterised in more detail using radial velocity follow-up observations. Not only is its size very similar to that of the Earth (1.2R⊕ ), it ...
Document
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... Water ice, dry ice, rocks, dirt, & gas (a dirty snowball) ...
So, what`s the problem for high
So, what`s the problem for high

... finished accretion from its parent cloud core. Radiation pressure should stop accretion before a star can reach its final mass. High-mass stars only form in clusters, so isolating individuals is difficult: Almost no HMPOs have been unambiguously identified at specific star-like points on the sky tha ...
Astro 7B – Solution Set 7 1 A Star is Born
Astro 7B – Solution Set 7 1 A Star is Born

... have two stars smash together. Another way to “collide” is for a star to gravitationally deflect the trajectory of another star — to change its direction by an angle on the order of, say, unity (i.e., ∼1 rad). We will work out the latter case. The timescale for a star to gravitationally deflect the ...
Lecture15_v1 - Lick Observatory
Lecture15_v1 - Lick Observatory

... The unmanned lunar probe Surveyor 3 soft-landed on the Moon in 1967. In 1969, 2.5 yrs later, Apollo12 astronauts Pete Conrad and Alan Bean recovered the camera from Surveyor 3 and brought it back to Earth. The insulation covering its circuit boards contained 50 to 100 viable specimens of Streptococc ...
Birth - Wayne State University Physics and Astronomy
Birth - Wayne State University Physics and Astronomy

... balances gravity. Fusion continues until most of the hydrogen in the core is used up. 29 March 2005 ...
Icy Bodies in the New Solar System - UCLA
Icy Bodies in the New Solar System - UCLA

... subsequent returns, thereby decreasing their number in any magnitude-limited plot. The “fading parameter” is really a “fudge parameter” needed to make the model fit the data, and the physical nature of the fading remains unspecified, although suggestions abound (Levison et al. 2002, Dones et al. 200 ...
Kepler Mission Workshop Presentation
Kepler Mission Workshop Presentation

... lava and much too hot for life as we know it • All five of the exoplanets orbit stars hotter and larger than Earth's sun. ...
Disk-planet interaction
Disk-planet interaction

... arguments about impossibility of other worlds, despite a growing controversy within Church. ...
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Directed panspermia

Directed panspermia concerns the deliberate transport of microorganisms in space to be used as introduced species on lifeless planets. Directed panspermia may have been sent to Earth to start life here, or may be sent from Earth to seed exoplanets with life.Historically, Shklovskii and Sagan (1966) and Crick and Orgel (1973) hypothesized that life on Earth may have been seeded deliberately by other civilizations. Conversely, Mautner and Matloff (1979) and Mautner (1995, 1997) proposed that we ourselves should seed new planetary systems, protoplanetary discs or star-forming clouds with microorganisms, to secure and expand our organic gene/protein life-form. To avoid interference with local life, the targets may be young planetary systems where local life is unlikely. Directed panspermia can be motivated by biotic ethics that value the basic patterns of organic gene/protein life with its unique complexity and unity, and its drive for self-propagation.Belonging to life then implies panbiotic ethics with a purpose to propagate and expand life in space. Directed panspermia for this purpose is becoming possible due to developments in solar sails, precise astrometry, the discovery of extrasolar planets, extremophiles and microbial genetic engineering. Cosmological projections suggests that life in space can then have an immense future.
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