Neutron Star facts
While investigating facts about Neutron Star Collision and Neutron Star Definition, I found out little known, but curios details like:
There's a type of neutron star called a magnetar which has a magnetic field that's so powerful that being within 1,000 miles of one would warp all the atoms in your body and from a distance of 100,000 miles away it would be able to wipe out the data of every credit card on the planet.
how neutron stars form?
A teaspoon of matter taken from a neutron star would weigh around 10 billion tons, which is similar to the weight of an average earth mountain.
What's neutron star?
In my opinion, it is useful to put together a list of the most interesting details from trusted sources that I've come across answering what neutron star made of. Here are 50 of the best facts about Neutron Star Drop and Neutron Star Density I managed to collect.
what happens at neutron star?
-
A neutron star's gravity is so immense, that the surface of the star is perfectly flat, and any 'protrusions' never exceed 5 mm. Also, neutron stars are usually around 13 km in diameter, yet a sugar cubed sized portion of the star would weigh more than Mt. Everest.
-
A neutron star is so dense that a matchbox sized portion of one would weigh 3 billion tons.
-
A shot glass filled with neutron star matter would weigh as much as Mount Everest.
-
A neutron star is so dense if you dropped a gummy bear from one meter above it would hit the surface in a nonosecond at around 7,000,000 KM/H with the force of 1,000 nuclear bombs.
-
The gravity of a neutron star is so strong that parts of the opposite side can be seen from the front, as light is bent around it.
-
The neutron star 'PSR J1748-2446ad' rotates on its axis 716 times per second, and is the fastest spinning known neutron star. At its equator, it spins at 24 percent of the speed of light.
-
Neutron star PSR J1748-2446 is the fastest spinning celestial object in the universe. The star rotates 716 times every second, so its equator moves at about 25% the speed of light. It is also 50 trillion times the density of lead and has a magnetic field a trillion times stronger than the Sun’s.
-
A neutron star's gravitational field is so strong, it bends light such that we can see more than half of its surface at once
-
The fastest known neutron star spins at 716 times a second, and their spin rates are extremely reliable - so accurate they even surpass atomic clocks as natures most precise timepieces.
Why neutron stars don't collapse?
You can easily fact check why neutron stars are pulsars by examining the linked well-known sources.
Gold is created by two neutron stars colliding
In 2004, a Magnetar (a type of a Neutron Star with a powerful magnetic field) had a large gamma ray burst which briefly expanded the ionosphere. It is thought to be the largest explosion observed in the galaxy by humans since the supernova observed by Johannes Kepler in 1604. - source
A neutron star is so dense if you dropped a gummy bear from one meter above the ground, it would hit the surface in a nanosecond at around 7,000,000 kilometers (about 4,349,598 miles) per hour with the force of 1,000 nuclear bombs. - source
If a marshmallow were dropped a foot above the surface of a neutron star it would have the same energy of a modern atomic bomb
When a star explodes into a supernova and it is not very big it can end up becoming a nebula and neutron star. A larger one may result in a black hole.
When neutron stars collide?
Neutron stars, despite being incredibly massive, rotate once per second - and can rotate even faster if they have a binary twin
How neutron stars die?
In 2004 a neutron star blasted earth with more radiation ever recorded, from 50,000 light years away.
Inside neutron stars, nuclear material can form "nuclear pasta", where it exists in phases like the spaghetti and lasagna phase, so named for their resemblance to pasta.
A magnetar is a highly magnetic neutron star. It has fields so magnetic that it can rip you apart from over 600 miles away.
One teaspoon of neutron star matter would weigh roughly one billion pounds.
The source was identified several years later as a rapidly rotating neutron star and was designated PSR B1919+21.