ar X iv : a st ro - p h / 02 08 55 6 v 3 2 3 Se p 20 02 Galactic Environment of the Sun and Stars : Interstellar and Interplanetary Material
نویسندگان
چکیده
Interstellar material surrounding an extrasolar planetary system interacts with the stellar wind to form the stellar astrosphere, and regulates the properties of the interplanetary medium and cosmic ray fluxes throughout the system. Advanced life and civilization developed on Earth during the time interval when the Sun was immersed in the vacuum of the Local Bubble and the heliosphere was large, and probably devoid of most anomalous and galactic cosmic rays. The Sun entered an outflow of diffuse cloud material from the Sco-Cen Association within the past several thousand years. By analogy with the Sun and solar system, the Galactic environment of an extrasolar planetary system must be a key component in understanding the distribution of systems with stable interplanetary environments, and inner planets which are shielded by stellar winds from interstellar matter (ISM), such as might be expected for stable planetary climates.
منابع مشابه
ar X iv : a st ro - p h / 02 08 55 6 v 2 3 0 A ug 2 00 2 Galactic Environment of the Sun and Stars : Interstellar and Interplanetary Material
Interstellar material surrounding an extrasolar planetary system interacts with the stellar wind to form the stellar astrosphere, and regulates the properties of the interplanetary medium and cosmic ray fluxes throughout the system. Advanced life and civilization developed on Earth during the time interval when the Sun was immersed in the vacuum of the Local Bubble and the heliosphere was large...
متن کاملar X iv : a st ro - p h / 02 08 55 6 v 1 3 0 A ug 2 00 2 Galactic Environment of the Sun and Stars : Interstellar and Interplanetary Material
Interstellar material surrounding an extrasolar planetary system interacts with the stellar wind to form the stellar astrosphere, and regulates the properties of the interplanetary medium and cosmic ray fluxes throughout the system. Advanced life and civilization developed on Earth during the time interval when the Sun was immersed in the vacuum of the Local Bubble and the heliosphere was large...
متن کاملar X iv : a st ro - p h / 01 09 30 0 v 1 1 8 Se p 20 01 Local Interstellar Matter : The view from Paris
Observations of interstellar gas and dust towards nearby stars and within the solar system show that the Sun is embedded in a warm diffuse partiallyionized cloud. This cloud is the leading edge of a flow of interstellar matter (ISM) through our Galactic neighborhood. Interstellar matter sets the boundary conditions of the heliosphere and astrospheres of extra-solar planetary systems. Moreover, ...
متن کاملar X iv : a st ro - p h / 02 09 19 6 v 1 1 0 Se p 20 02 Preliminary Abundance Analysis of Galactic Bulge Main Sequence , Subgiant , and Giant Branch Stars Observed
We present an abundance analysis of six main sequence turnoff, subgiant, and giant branch stars toward the Galactic bulge that were observed with Keck/HIRES during microlensing events. This is an early look at the first detailed chemical analysis of main sequence stars in the Galactic bulge. Lensing events allow the effective aperture of Keck to be increased beyond its current dimensions; altho...
متن کاملar X iv : a st ro - p h / 07 02 59 6 v 3 2 5 M ay 2 00 7 The Local Bubble and Interstellar Material Near the Sun
The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in...
متن کاملذخیره 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 2002