Scientists using the IceCube Observatory located near the South Pole have discovered that neutrinos can be absorbed by our Planet Earth. With almost no mass and no charge, these particles rarely interact with matter. Yet tens of trillions of neutrinos pass through our bodies every second. Previous theories predicted that at high energies, neutrinos can be expected to interact with matter and be absorbed by the Earth instead of passing through the planet. “We knew that lower-energy neutrinos pass through just about anything, but although we had expected higher-energy neutrinos to be different, no previous experiments had been able to demonstrate convincingly that higher-energy neutrinos could be stopped by anything,” said Penn State Professor Doug Cowen. “However, the neutrino does have a tiny probability to interact, and this probability increases with energy. That probability is what scientists call the neutrino cross section.” The new measurements recorded by IceCube determined the neutrino cross section energies to be about 6.3 TeV and 980 TeV, energy levels significantly higher than previously measured.
Read more about this fascinating story at: http://www.newsoftheuniverse.com/2017/11/cosmic-neutrinos-can-be-absorbed-by.html
Taurus constellation
(ESA/Hubble) Hubble-X is a glowing gas cloud, one of the most active star-forming regions within galaxy NGC 6822. The name Hubble-X does not refer to the shape of the gas cloud, but rather is derived from a catalog of objects in this particular galaxy.
Credit: NASA/ESA and The Hubble Heritage Team (STScI/AURA)
About the Object Name: Barnard’s Galaxy, Hubble-X, NGC 6822 Type: Local Universe : Nebula : Type : Star Formation Local Universe : Galaxy : Type : Barred Local Universe : Galaxy : Type : Irregular Distance: 2 million light years ConstellatioSagittarius Category: Galaxies
Coordinates
Position (RA):19 45 5.03 Position (Dec): -14° 43’ 20.00" Field of view: 1.09 x 1.01 arcminutes Orientation: North is 305.8° left of vertical
Source
Astronomers using the Atacama Large Millimeter/millimeter Array (ALMA) in Chile have discovered two giant galaxies that existed when the universe was only 780 million years old, or about 5 percent of its current age. These two galaxies, known collectively as SPTO311-58, appear to be within an even-more-massive dark matter halo, containing several trillion times the mass of our sun. This discovery is quite surprising for scientists. Like how suns and planets are formed from clumps of gas and rock sticking together, astronomers expected the first galaxies to resemble little dwarf galaxies such as those seen today. Yet, nature has surprised everybody, revealing examples of massive galaxies - even for today’s standards. The researchers wrote the following statement: “This ‘de-lensing’ process provided intriguing details about the galaxies, showing that the larger of the two is forming stars at a rate of 2,900 solar masses per year. It also contains about 270 billion times the mass of our sun in gas and nearly 3 billion times the mass of our sun in dust.” This shows that these galaxies very likely merged to eventually form the largest galaxy ever observed at that time period in cosmic history.
Read more about this fascinating story at: http://earthsky.org/space/primordial-galaxies-spt0311-58-dark-matter-early-universe
Images: Artist’s concept via NRAO/ AUI/ NSF; D. Berry. & Composite Image via ALMA (ESO/NAOJ/NRAO), Marrone, et al.; B. Saxton (NRAO/AUI/NSF); NASA/ESA Hubble.
NGC 2170