- published: 07 May 2015
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In astronomy, the interstellar medium (ISM) is the matter that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. The energy that occupies the same volume, in the form of electromagnetic radiation, is the interstellar radiation field.
The interstellar medium is composed of multiple phases, distinguished by whether matter is ionic, atomic, or molecular, and the temperature and density of the matter. The interstellar medium is composed primarily of hydrogen followed by helium with trace amounts of carbon, oxygen, and nitrogen comparatively to hydrogen. The thermal pressures of these phases are in rough equilibrium with one another. Magnetic fields and turbulent motions also provide pressure in the ISM, and are typically more important dynamically than the thermal pressure is.
Voyager 1 is a space probe launched by NASA on September 5, 1977. Part of the Voyager program to study the outer Solar System, Voyager 1 launched 16 days after its twin, Voyager 2. Having operated for 38 years, 5 months and 12 days, the spacecraft still communicates with the Deep Space Network to receive routine commands and return data. At a distance of 134 AU (2.00×1010 km) as of winter 2016, it is the farthest spacecraft from Earth and the only one in interstellar space.
The probe's primary mission objectives included flybys of Jupiter, Saturn, and Saturn's large moon, Titan. While the spacecraft's course could have been altered to include a Pluto encounter by forgoing the Titan flyby, exploration of the moon, which was known to have a substantial atmosphere, took priority. It studied the weather, magnetic fields, and rings of the two planets and was the first probe to provide detailed images of their moons.
After completing its primary mission with the flyby of Saturn on November 20, 1980, Voyager 1 began an extended mission to explore the regions and boundaries of the outer heliosphere. On August 25, 2012, Voyager 1 crossed the heliopause to become the first spacecraft to enter interstellar space and study the interstellar medium. Voyager 1's extended mission is expected to continue until around 2025, when its radioisotope thermoelectric generators will no longer supply enough electric power to operate any of its scientific instruments.
Voyager may refer to:
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In this video, we explore what lies between the stars, the interstellar medium. What is it? Why is it significant? Enter the Evant Horizon and find out! -photos by NASA Connect with me: Facebook: http://on.fb.me/1LfbEk5 Twitter: https://twitter.com/_evanthorizon_ Instagram: https://instagram.com/evanthorizon Tumblr: http://cosmicevanthorizon.tumblr.com/ Pinterest: https://www.pinterest.com/Evanthorizon/
Source - http://serious-science.org/videos/1278 University of California, Berkeley Prof. Christopher McKee on giant molecular clouds, hot gas in the halo of the Galaxy, and dominant heating mechanism
Dr. Michelle Thaller explains how there can be an interstellar medium in a vacuum.
This minilecture discusses the oft-invisible gas and dust found between stars, the interstellar medium. We discuss how this material can be detected as a nebula and the most common types of nebulae. Table of Contents: 00:00 - Introduction 00:45 - The Circle of Life 01:54 - The Circle of (Star) Life 03:00 - The struggle between gravity and pressure 03:40 - The space between stars is not empty, but is full of gas and dust, called the interstellar medium. 04:21 - Illuminating the material between stars 05:42 - Time-lapse view of V838 Monoceratis 07:04 - Types of nebulae 07:53 - Reflection nebulae 10:21 - Emission nebulae 11:04 - Star-forming Nebulae 11:39 - Planetary Nebulae 13:02 - Supernova Remnants 13:54 - Dark Nebulae 16:54 - Summary: Types of Nebulae
NASA's Voyager 1 spacecraft made history in 2012 by entering interstellar space, leaving the planets and the solar wind behind. But observations from the pioneering probe were puzzling with regard to the magnetic field around it, as they differed from what scientists derived from observations by other spacecraft. A new study offers fresh insights into this mystery. Writing in the Astrophysical Journal Letters, Nathan Schwadron of the University of New Hampshire, Durham, and colleagues reanalyzed magnetic field data from Voyager 1 and found that the direction of the magnetic field has been slowly turning ever since the spacecraft crossed into interstellar space. They believe this is an effect of the nearby boundary of the solar wind, a stream of charged particles that comes from the sun. ...
Professor Mike Brown from Caltech presents "Exploring in the Interstellar Medium" during the short course at the Keck Institute for Space Studies on September 8, 2014. In conjunction with the KISS program "Science and Enabling Technologies to Explore the Interstellar Medium"
This year’s Rosseland Lecture was held by Anja C. Andersen, associate Professor at Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen. Dust grains are found everywhere in the space between the stars in galaxies. They are responsible for the formation of molecular hydrogen and for absorbing and re-emitting about 50% of the energy from all galaxies, as well as providing an effective coolant for star formation. Although important in various astrophysical processes, the origin and consequently the chemical make-up and emission properties of dust grains is largely unknown. Dust is generally believed to form in the atmospheres of low/intermediate-mass stars late in life, but there is growing evidence that dust may also be formed in the explosions of massive stars and/or be ac...
In astronomy, the "interstellar medium" is the matter that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. The energy that occupies the same volume, in the form of electromagnetic radiation, is the "interstellar radiation field". The interstellar medium is composed of multiple phases, distinguished by whether matter is ionic, atomic, or molecular, and the temperature and density of the matter. The interstellar medium is composed primarily by hydrogen followed by helium with trace amounts of carbon, oxygen, and nitrogen comparatively to hydrogen. The thermal pressures of these phases are in ro...
ASTRONOMY TODAY (Chaisson, McMillan) - CHAPTER 18
http://www.SpaceChronology.com Courtesy NASA/JPL-Caltech/Spitzer Telescope