On Nuking Menacing Asteroids

نویسنده

  • K A Holsapple
چکیده

Introduction: Most scientists now accept that impacts on the earth of large asteroids and comets have occurred in the past, and will, without intervention , occur again; with devastating affects on the earth and all living creatures. About ten years ago, researchers [1,2] and others studied a number of ways that an asteroid could be diverted from an impending collision with the earth by pushing it sufficiently to change its course, making it miss the earth. Among the methods suggested, it is generally accepted that with a short warning time, such as a few years, only the nuclear bomb approach would work. In [3] I report some recent studies on these issues, including the effect of asteroid porosity which is now thought to be likely. One of the conclusions is that porosity can make the use of surface explosives or impacts of large masses, both methods that deflect by cratering, ineffective. Of the other cases, some of the more interesting conclusions deal with the mitigation methods using a standoff nuclear weapon, which I present here. Deflection by standoff nuclear detonations: The standoff method uses a nuclear weapon detonated at some height above the asteroid surface, resulting in a large deposition of x-ray or neutron energy into a surface layer of the asteroid. The neutrons penetrate further so generally give more effect than the x-rays. Therefore I assume a weapon designed for a significant neutron yield. Both [1] and [2] consider this method. Both obtain estimates of the impulse imparted to the asteroid by estimating a blow-off velocity and a total blow-off mass. A more precise result is obtained by an analysis of the wave dynamics of the processes, which I obtained using a one-dimensional wave propagation code and the ANEOS three phase equation of state for the response of the asteroid material. I consider both porous and non-porous materials. I use the ANEOS model for Quartz given in [5]. For the porous case, the Herrmann p-alpha model is added to the underlying EOS for quartz. The p-alpha model is characterized by three material properties. The distension ratio α is the porous mass density divided by the mass density of the particulate solid material. The pressure P e is a pressure at which crush begins, and P s the pressure at which all voids are crushed out. There is a curve of distension v. pressure defined by these three parameters. To …

برای دانلود رایگان 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

Physical models of asteroids from sparse photometric data

We present an overview of our work on shape and spin state determination of asteroids from photometric data sparse in time. Our results are based on simulations that were performed using realistic shape and light-scattering models and time sequences that will be provided by Pan-STARRS (Panoramic Survey Telescope and Rapid Response System). We show some typical examples of physical model reconst...

متن کامل

Production of Cosmic Dust by Hydrous and Anhydrous Asteroids: Implications for the Production of Interplanetary Dust Particles and Micrometeorites. G

Introduction: In our Solar System the asteroid belt is compositionally zoned, with the asteroids similar in reflection spectrum to the carbonaceopus meteorites dominating the outer-half of the main belt. In the outer-half of the main belt about one-half of the carbonaceous asteroids are hydrous, based on their infrared spectra [1]. The asteroids in the inner-half of the main belt are predominan...

متن کامل

Inelastic Dissipation in Wobbling Asteroids and Comets

Asteroids and comets dissipate energy when they rotate about any axis different from the axis of the maximal moment of inertia. We show that the most efficient internal relaxation happens at twice the frequency of the body’s precession. Therefore earlier estimates that ignore the double frequency input underestimate the internal relaxation in asteroids and comets. We suggest that the Earth’s se...

متن کامل

Eclipse Prediction and Orbit Improvement for Asteroids: Theory and Application to Near Earth Asteroids

Asteroids can be eclipsed by other bodies in the Solar System, but no direct observation of an asteroid eclipse has been reported to date. We describe a statistical method to predict an eclipse for an asteroid based on the analysis of the orbital elements covariance matrix. By propagating a set of Virtual Asteroids to an epoch correspondent to a close approach with a Solar System planet or natu...

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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003