Dark Energy

"Night Sky"

La Vía Láctea sobre Dead Vlei en el desierto de Namib en Namibia.

Panorama de 3 fotos individuales: Sony A75 l Sigma mm F / 1 .8 || s l IS0 5000

Crédito: Stefan Liebermann

https://instagram.com/stefanliebermannphoto

https://www.stefanliebermann.de/

~Antares

Lanzamiento del telescopio "X-ray Polarimetry Explorer" (IXPE) en el Falcon 9 de SpaceX, cuyo objetivo es estudiar los rayos X liberados por los agujeros negros y estrellas de neutrones.

Crédito: Matt Cutshall

https://instagram.com/booster_buddies

https://twitter.com/Booster_Buddies

https://nexthorizonsspaceflight.com

~Antares

Luna

La imagen ganadora presentada fue tomada sobre el lago glacial más grande de Islandia . El fotógrafo combinó seis exposiciones para capturar no solo dos anillos de auroras verdes , sino también sus reflejos en el lago sereno. Visible en el cielo de fondo distante es la banda de nuestra Vía Láctea y la galaxia de Andrómeda .

Créditos: Stephane Vetter

Cerca de un equinoccio, el campo magnético de la Tierra está orientado a favorecer las interacciones con el viento solar que desencadenan el atractivo resplandor de la aurora boreal. En los cielos sobre Kaunispää Hill, Laponia, Finlandia.

Créditos: Juan Carlos Casado (TWAN, Tierra y estrellas)

Auroras boreales en Finlandia. ¿Te gustaría saber más información de este tipo de fenómenos? En este video te lo explicamos:

https://youtu.be/ucbLpiGVWiU

Crédito: Ryan Oliveira

https://instagram.com/roliveira33

~Antares

Descubrir los errores de otros, tarea que para la naturaleza humana es mucho más fácil que percibir los errores propios.

This is the Hyades Cluster! ✨✨✨

As the closest star cluster to Earth, this star cluster contains hundreds of stars with some of the brighter ones in this image transforming into giant stars as they enter a new phase of their lifespan. Some theorize that the creation of this cluster may have happened all at once as many of these stars are the same age and move in a similar way! 💫💫💫

Taken by me (Michelle Park) using the Slooh Canary Two telescope on November 6th, 2020 at 22:15 UTC.

What’s Inside a ‘Dead’ Star?

Matter makes up all the stuff we can see in the universe, from pencils to people to planets. But there’s still a lot we don’t understand about it! For example: How does matter work when it’s about to become a black hole? We can’t learn anything about matter after it becomes a black hole, because it’s hidden behind the event horizon, the point of no return. So we turn to something we can study – the incredibly dense matter inside a neutron star, the leftover of an exploded massive star that wasn’t quite big enough to turn into a black hole.

Our Neutron star Interior Composition Explorer, or NICER, is an X-ray telescope perched on the International Space Station. NICER was designed to study and measure the sizes and masses of neutron stars to help us learn more about what might be going on in their mysterious cores.

When a star many times the mass of our Sun runs out of fuel, it collapses under its own weight and then bursts into a supernova. What’s left behind depends on the star’s initial mass. Heavier stars (around 25 times the Sun’s mass or more) leave behind black holes. Lighter ones (between about eight and 25 times the Sun’s mass) leave behind neutron stars.

Neutron stars pack more mass than the Sun into a sphere about as wide as New York City’s Manhattan Island is long. Just one teaspoon of neutron star matter would weigh as much as Mount Everest, the highest mountain on Earth!

These objects have a lot of cool physics going on. They can spin faster than blender blades, and they have powerful magnetic fields. In fact, neutron stars are the strongest magnets in the universe! The magnetic fields can rip particles off the star’s surface and then smack them down on another part of the star. The constant bombardment creates hot spots at the magnetic poles. When the star rotates, the hot spots swing in and out of our view like the beams of a lighthouse.

Neutron stars are so dense that they warp nearby space-time, like a bowling ball resting on a trampoline. The warping effect is so strong that it can redirect light from the star’s far side into our view. This has the odd effect of making the star look bigger than it really is!

NICER uses all the cool physics happening on and around neutron stars to learn more about what’s happening inside the star, where matter lingers on the threshold of becoming a black hole. (We should mention that NICER also studies black holes!)

Scientists think neutron stars are layered a bit like a golf ball. At the surface, there’s a really thin (just a couple centimeters high) atmosphere of hydrogen or helium. In the outer core, atoms have broken down into their building blocks – protons, neutrons, and electrons – and the immense pressure has squished most of the protons and electrons together to form a sea of mostly neutrons.

But what’s going on in the inner core? Physicists have lots of theories. In some traditional models, scientists suggested the stars were neutrons all the way down. Others proposed that neutrons break down into their own building blocks, called quarks. And then some suggest that those quarks could recombine to form new types of particles that aren’t neutrons!

NICER is helping us figure things out by measuring the sizes and masses of neutron stars. Scientists use those numbers to calculate the stars’ density, which tells us how squeezable matter is!

Let’s say you have what scientists think of as a typical neutron star, one weighing about 1.4 times the Sun’s mass. If you measure the size of the star, and it’s big, then that might mean it contains more whole neutrons. If instead it’s small, then that might mean the neutrons have broken down into quarks. The tinier pieces can be packed together more tightly.

NICER has now measured the sizes of two neutron stars, called PSR J0030+0451 and PSR J0740+6620, or J0030 and J0740 for short.

J0030 is about 1.4 times the Sun’s mass and 16 miles across. (It also taught us that neutron star hot spots might not always be where we thought.) J0740 is about 2.1 times the Sun’s mass and is also about 16 miles across. So J0740 has about 50% more mass than J0030 but is about the same size! Which tells us that the matter in neutron stars is less squeezable than some scientists predicted. (Remember, some physicists suggest that the added mass would crush all the neutrons and make a smaller star.) And J0740’s mass and size together challenge models where the star is neutrons all the way down.

So what’s in the heart of a neutron star? We’re still not sure. Scientists will have to use NICER’s observations to develop new models, perhaps where the cores of neutron stars contain a mix of both neutrons and weirder matter, like quarks. We’ll have to keep measuring neutron stars to learn more!

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