High Resolution Pictures

Water ice clouds on Mars (desktop/laptop) Click the image to download the correct size for your desktop or laptop in high resolution

Ice desert by JustV23

Earth-Like World

Picture of the Day 2 - October 16, 2018

Here I come across the most Earth-like planet to date. The planet is covered in green vegetation, blue oceans and ice caps at the poles. This planet is located near the galactic core; therefore, the sky is full of bright stars, even more so than globular clusters.

Picture of the day - December 18, 2018

Polar vortex over the northern pole of Insight A-II

Picture of the Day 2 - November 9, 2018

Narrow sea cuts through the forests of a life supporting world with red-colored vegetation.

Triangulum Log - Post 1 - The Outskirts.

My first adventure brings us to this Yellow Super Giant and companion black hole. The system is young and filled with many gas giants that still glow with the heat of their formation.

All of the planets orbit far from the star, the nearest having a orbital radius of 10.57 AU. Numerous planets are also double planets including a double Jupiter as shown above.

More pics of this system and my thoughts on if this system could actually exist in the real universe to come.

Picture of the day 2 - November 25, 2018

More moons. A small and large moon orbiting a ringed gas-giant. The bright star transited by the rings is a nearby bright giant, but not part of this planet’s star system.

Using All of Our Senses in Space

Today, we and the National Science Foundation (NSF) announced the detection of light and a high-energy cosmic particle that both came from near a black hole billions of trillions of miles from Earth. This discovery is a big step forward in the field of multimessenger astronomy.

But wait — what is multimessenger astronomy? And why is it a big deal?

People learn about different objects through their senses: sight, touch, taste, hearing and smell. Similarly, multimessenger astronomy allows us to study the same astronomical object or event through a variety of “messengers,” which include light of all wavelengths, cosmic ray particles, gravitational waves, and neutrinos — speedy tiny particles that weigh almost nothing and rarely interact with anything. By receiving and combining different pieces of information from these different messengers, we can learn much more about these objects and events than we would from just one.

Lights, Detector, Action!  

Much of what we know about the universe comes just from different wavelengths of light. We study the rotations of galaxies through radio waves and visible light, investigate the eating habits of black holes through X-rays and gamma rays, and peer into dusty star-forming regions through infrared light.

The Fermi Gamma-ray Space Telescope, which recently turned 10, studies the universe by detecting gamma rays — the highest-energy form of light. This allows us to investigate some of the most extreme objects in the universe.

Last fall, Fermi was involved in another multimessenger finding — the very first detection of light and gravitational waves from the same source, two merging neutron stars. In that instance, light and gravitational waves were the messengers that gave us a better understanding of the neutron stars and their explosive merger into a black hole.

Fermi has also advanced our understanding of blazars, which are galaxies with supermassive black holes at their centers. Black holes are famous for drawing material into them. But with blazars, some material near the black hole shoots outward in a pair of fast-moving jets. With blazars, one of those jets points directly at us!

Multimessenger Astronomy is Cool

Today’s announcement combines another pair of messengers. The IceCube Neutrino Observatory lies a mile under the ice in Antarctica and uses the ice itself to detect neutrinos. When IceCube caught a super-high-energy neutrino and traced its origin to a specific area of the sky, they alerted the astronomical community.

Fermi completes a scan of the entire sky about every three hours, monitoring thousands of blazars among all the bright gamma-ray sources it sees. For months it had observed a blazar producing more gamma rays than usual. Flaring is a common characteristic in blazars, so this did not attract special attention. But when the alert from IceCube came through about a neutrino coming from that same patch of sky, and the Fermi data were analyzed, this flare became a big deal!

IceCube, Fermi, and followup observations all link this neutrino to a blazar called TXS 0506+056. This event connects a neutrino to a supermassive black hole for the very first time.  

Why is this such a big deal? And why haven’t we done it before? Detecting a neutrino is hard since it doesn’t interact easily with matter and can travel unaffected great distances through the universe. Neutrinos are passing through you right now and you can’t even feel a thing!

The neat thing about this discovery — and multimessenger astronomy in general — is how much more we can learn by combining observations. This blazar/neutrino connection, for example, tells us that it was protons being accelerated by the blazar’s jet. Our study of blazars, neutrinos, and other objects and events in the universe will continue with many more exciting multimessenger discoveries to come in the future.

Want to know more? Read the story HERE.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

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Picture of the Day 2 - January 16, 2019

A planet and it's moon burn under the glare of 4 suns.

Space Engine System ID: RS 8550-3584-5-403-110 B1.1