NEOWISE: the next nine nights
NEOWISE: die nächsten neun Nächte
22. Jul Verfasst von skyweek
#SPMN231021 recorded today at 1h44m55s TU (3h44m local time). This video captured from Estepa, Seville by Antonio J. Robles
@AJ_Robles. This small rock from Comet 2P / Encke broke apart in the atmosphere without producing meteorites. Soon on the list
Discovery Comet 2P/Encke was first discovered by Pierre F. A. Mechain on Jan. 17, 1786. Other astronomers located this comet in subsequent passages, but these sightings were not defined as the same comet until Johann Franz Encke calculated its orbit. Overview Comet 2P/Encke is a small comet. Its...
solarsystem.nasa.gov
#SPMN221021E recorded last night flying over the province of
#Salamanca at 19h19m34s (21h19m local time). Video captured by Antonio J. Robles
@AJ_Robles from Estepa, Seville. A faint aggregate of Comet 3D / Biela: Andromedida. Details:
http://spmn.uji.es/ESP/SPMNlist.h LAST BOLIDOS REGISTERED BY THE SPMN NETWORK
A snip of a long comprehensive post.
The most luminous shooting stars, those that equal or exceed the planet Venus (brightness magnitude -4 or less) are called the bolid or fireball . These phenomena are produced when a rock of interplanetary origin penetrates the Earth's atmosphere at speeds between 11 and 73 km / s. They are usually rocks detached from asteroids, comets or, more rarely, from the Moon or Mars.
From the Research Network on Bolids and Meteorites we study these phenomena since they inform about the arrival of meteorites, valuable samples of innumerable bodies of the Solar System. Below you will find a list of the most luminous bolides registered over Spain this year, and at the end there is a link to lists of previous years (since they began to be systematically registered by our network in 1999). This list is intended to be exhaustive (except for errors or omissions) for all the bolides whose brightness magnitude has been less than -7 (this is 16 times greater than the luminosity of the planet Venus). -12 magnitude bolids would have the luminosity of the full Moon and would already be at the limit of generating meteorites that, normally, tend to be tens or hundreds of times more luminous.
The following annual list also gives a scientific explanation to the bolides, given that in the "origin" sectionit is indicated if its origin is associated with some meteoric swarm or if, on the contrary, it is "sporadic" (not associated with a swarm or that it has lost its orbital kinship with its parent body).
Constantly rocks whose size ranges from centimeters to a few meters in diameter reach the Earth from the main asteroid belt as a consequence of gravitational disturbances with the planets as you can read in thisConstantly rocks whose size ranges from centimeters to a few meters in diameter reach the Earth from the main asteroid belt as a consequence of gravitational disturbances with the planets as you can read in this Constantly rocks whose size ranges from centimeters to a few meters in diameter reach the Earth from the main asteroid belt as a consequence of gravitational disturbances with the planets as you can read in thisinformative article .
Maintaining this page is a huge challenge, but it allows a rational explanation to be given to these luminous phenomena. This work is maintained thanks to a joint effort given that currently our hundred detectors cover about 95% of the Iberian Peninsula from more than 30 automatic and digital detection stations that operate every day of the year. or. Given this wide coverage, we annually detect more than 500 bolids, although statistically it is estimated that annually less than a dozen could produce meteorites in the Iberian Peninsula (1 or 2 with a mass greater than one kilogram). The detailed study of the trajectories of these fireballs allows us to determine in those cases the possible places of meteorite fall, although their recovery is not always feasible due to the intrinsic difficulties of each place. On the other hand, by determining their heliocentric orbits we can deduce their origin in the Solar System. All these results are published inprestigious magazines where we collect the gratitude to the visual testimonies or photographs that they send us. It is everyone's job to ensure that these luminous phenomena are properly and scientifically interpreted to develop the pseudoscience of our country.
Snip:
"In the heavens above, it's raining dirt.
Every second, millions of pieces of dirt that are smaller than a grain of sand strike Earth's upper atmosphere. At about 100 kilometers altitude, bits of dust, mainly debris from asteroid collisions, zing through the sky vaporizing as they go 10 to 100 times the speed of a bullet. The bigger ones can make streaks in the sky, meteors that take our breath away.
Scientists are using supercomputers to help understand how tiny meteors, invisible to the naked eye, liberate electrons that can be detected by radar and can characterize the speed, direction and rate of meteor deceleration with high precision, allowing its origin to be determined. Because this falling space dust helps seed rain-making clouds, this basic research on meteors will help scientists more fully understand the chemistry of Earth's atmosphere. What's more, meteor composition helps astronomers characterize the space environment of our solar system".
Canada
Event
AMS #6843-2021
https://youtu.be/tey8cCaGyjg
Oct 23, 2021
Oct 23, 2021