M City

[Guayota 🏴󠁧󠁢󠁳󠁣󠁴󠁿 ⭐ ⭐ @IIllllllIlIIllI]

Ganaron 12 Copas de América antes de 1959, con torneos de solo 3 o 4 selecciones.
Desde ese año, solo han levantado 4 trofeos más. Cuatro.
Eurocopas se han jugado 17 y Copas de América 48 ediciones.

Seguiré repitiéndolo todo lo que haga falta para ponerlo en contexto.

[Nahuel 1000  🇦🇷 @RealGOA7]

Me encanta que te DUELA,
Me encanta que te ARDA,
Me encanta que lo VEAS.

Somos tan ARGENTINOS como
DIEGO ARMANDO MARADONA,
y SÍ, RESPETAMOS y ADMIRAMOS a
CRISTIANO RONALDO DOS SANTOS AVEIRO

Aunque te DUELA,
Aunque te ARDA,
Aunque NO lo entiendas JAMÁS

El único enemigo SOS VOS.

[Javier Rubio Donzé @Sr_Donze]

Este es, quizás, el vídeo más descarado de la Final de la Copa del Mundo. Todos vimos cómo Enzo Fernández casi mata a Pau Cubarsí, pero si te fijas, más abajo, un jugador de Argentina, Nicolás Tagliafico, ve la tremenda patada de su compañero y, sabiendo que la ha cagado, se le ocurre tirarse al suelo y fingir una lesión. Enzo recibe la tarjeta roja, pero Messi se acerca al árbitro señalando a su compañero argentino caído (a Tagliafico) diciendo que está lesionado. Afortunadamente no coló. Son delincuentes, no jugadores de fútbol.

[Matt Reeves @mattreevesLA]

https://t.co/O0TdgldMdK

[` @chixxsays]

This edit deserves an Oscar 🥹❤️ https://t.co/90cCld0BJz

[Ryanair @Ryanair]

not with VARgentina

[Cristiano Ronaldo @Cristiano]

Portugal Sempre

[Gobierno de México @GobiernoMX]

#MañaneraDelPueblo | La presidenta @Claudiashein reafirma el apoyo de México al pueblo de Venezuela; anuncia la asistencia de rescatistas de la Secretaría de la Defensa Nacional y personal de salud, luego de los sismos registrados este miércoles.

[Erika  @ExploreCosmos_]

Galaxies don’t have a simple maximum size because they don’t have sharp physical edges. Unlike planets or moons, a galaxy gradually fades outward: its stars, gas and dark matter become more diffuse until they blend into the background sky.

That makes “size” partly a measurement problem.

Astronomers often define a galaxy’s visible boundary using surface brightness, meaning how much light the galaxy contributes over a small patch of sky compared with the surrounding background. This works reasonably well, but it is still somewhat arbitrary, especially for faint outer disks, halos and elliptical galaxies.

Distance adds another complication: a galaxy can be physically enormous but look small because it is very far away, so astronomers need redshift and distance estimates to infer its true scale.

The Milky Way is already a large spiral galaxy, with a stellar disk at least about 100,000 light-years across, but it is far from the largest known galaxy. Some giant spiral galaxies are much wider.

Malin 1, for example, looked at first like a fairly ordinary spiral, but deep observations revealed extremely faint outer spiral structures extending across about 650,000 light-years. That makes it roughly six times wider than the Milky Way and one of the largest known spiral galaxies.

Another example is UGC 2885, also called Rubin’s Galaxy, which is nearly 450,000 light-years wide and contains far more stars than the Milky Way. These galaxies are puzzling because they seem relatively isolated, so their huge size can’t easily be explained by recent violent interactions with many neighboring galaxies. One possibility is that they grew through older or gentler mergers that no longer leave obvious distortions.

Collisions can also make galaxies appear huge by pulling out long tidal tails, as happens in systems such as the Tadpole Galaxy or the Condor Galaxy. But these stretched shapes are temporary phases, not necessarily stable examples of how large an ordinary galaxy can become.

Elliptical galaxies can grow even larger than spirals, especially near the centers of galaxy clusters, where repeated mergers are common. Some central elliptical galaxies can span more than a million light-years; ESO 383-76, for instance, is described as about 1.8 million light-years wide.

There are also giant isolated ellipticals, such as ESO 306-17, which may be the final product of many galaxies in a smaller cluster merging into one enormous object.

The main conclusion is that there is no known hard upper limit yet. The largest galaxies are hard to detect because their outer regions can be extremely faint and diffuse. Future wide-field observatories, especially the Vera C. Rubin Observatory and the Nancy Grace Roman Space Telescope, should be able to find more low-surface-brightness giants and help astronomers understand whether the biggest galaxies we know are close to the true limit, or whether even larger, dimmer galaxies are still hidden in the data.

[M City @AstroM198]

@NiTanTetonaa Soy Molotov

Sólo te digo que están tratando de doxearte y te están utilizando, usando tu acusación contra mi de hace un año para tratar de molestarme nuevamente

Que tú le estás dando información y demás...

[M City @AstroM198]

@ipoolgian @NoMercyVenz @Andrea_Ch_16 @KuroNoRoninn @cristiancrespoj @AnonymousVene10 @dragondrakarys1 @soldadoDfranela @TheMatrixNM @HackingTeam777 @Anon0tp0r @NiTanTetonaa

[M City @AstroM198]

@quemalandrita @locoincorrectos Espero estés lista para la futura demanda, Andrea

[M City @AstroM198]

📹: Chris Henry

[M City @AstroM198]

🇻🇪 Canaima

📹: @luke_jclark

[M City @AstroM198]

🇬🇧 London

📸: Luke Stackpoole

[M City @AstroM198]

🇳🇴 Måtind, Bleik

📹: janisview

[M City @AstroM198]

🏴󠁧󠁢󠁳󠁣󠁴󠁿 Edinburg, Scotland

📸: Cuma Cevik

[M City @AstroM198]

🇺🇸 The Roosevelt Island Tramway, NYC