Why are Saturn’s poles geometric? Saturn’s North Pole has been known to be surrounded by a hexagonal (6 sides) cloud since discovery in 1987 in data taken by NASA’s Voyager spacecrafts, which quickly flew past the ringed world in the early 1980s. Now, recent observations of Saturn by the Hubble Space Telescope reveal a slightly different geometric cloud pattern around the South Pole: a decagon (10 sides). The geometric boundaries are possibly caused by waves when the fast-moving gas away from the poles interacts with slower-moving gas closer to the poles. In the featured image composite by the Hubble taken last year, the South Pole of Saturn is marked by an X and surrounded by bands of circulating clouds. The decagon appears most prominent in the dark inner regions. The northern hexagon has proven stable for over 40 years, while the stability of the southern decagon will surely remain a topic of research.
Image Credit: NASA, ESA, STScI, HST; A. Sánchez-Lavega (UPV), A. Simon (NASA-GSFC), M. Wong (UC Berkeley); Processing: A. Pagan (STScI)
Is this star winking at us?
The central object in today’s animation is not one but two stars. XZ Andromedae, indicated by the bold lines, is an Algol-type eclipsing binary with a nearly edge-on orbit from Earth’s perspective.
The bottom light curve shows the amount of light from the system dim and brighten as the cooler star eclipses its hotter, brighter companion. Analysis of several XZ Andromedae light curves indicates there may be two other stars orbiting the system.
This particular light curve was created with Citizen Astronomy, an open-source software for differential photometry.
The software takes the difference in brightness between a target and comparison star and traces its behavior over time.
This technique reduces most variations from the instrument and Earth’s atmosphere. In addition to eclipsing binaries, this analysis is useful for studying transiting exoplanets, accreting black holes, supernovae, and many more time-varying astronomical phenomena. Astrophotographers: try it out on your own data!
Video Credit: Ogetay Kayali (MTU, Starfront Observatories)
Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)
Gas + gravity + time leads to amazing results.
Look at this peculiar galaxy pair, NGC 7253. Gravity caused a couple hundred billion balls of hydrogen to light up as stars, held together in two great swarms that then collided, scattered & reassembled.
https://t.co/aNtzshyIAp
Eris is actually 25.7% heavier than Pluto.
It has a shiny white surface, while its moon Dysnomia, a quarter of its size, is very dark with an albedo of just 0.05.
This strange pair orbits between 38.1 and 97.49 AU from the Sun.
📡 “Betelgeuse's atmosphere is becoming spotty and asymmetric—and a nearby companion could be shaping the pattern” by @physorg_com
https://t.co/W41sXpho0N
Star Formation Winding Down 🌌
The Andromeda galaxy shines with stars, but star formation has been declining for the past 500 million years. Using @nasahubble data, scientists measured about 200 million stars to learn about the galaxy’s past activity.
https://t.co/61tztN2J8s
This animation shows the same star field photographed more than 100 years apart, in 1889 and 1991. Somewhere within the two green boxes, among thousands of stars, lies the source of the Wow! Signal. #AreciboWow
NEWS 🚨: NASA’s Roman Space Telescope is ready for liftoff tomorrow at 7:26 a.m. EDT
It will hunt for new exoplanets with a field of view 100 times larger than Hubble’s
Incredible: A Hubble capture of the overlapping spiral galaxies SDSS J115331 and LEDA 2073461, more than a billion light-years away!
(Credit: ESA/Hubble & NASA, W. Keel)
Mimas is a satellite of Saturn with a diameter of 396 km. Its low density, 1.15 g/cm3, indicates that it’s composed of water ice with a small amount of rock and -may be- a liquid ocean under its surface. It’s heavily cratered: Herschel is a crater of 139 km across.
Image: Cassini
Amazing: Evidence of flowing liquid on the surface of Pluto. Pluto!
The fluid is probably liquid nitrogen. In every environment, it seems, some elements or compounds behave in dynamic ways, producing active geology from Mercury to Pluto (and beyond?).
https://t.co/4lyW8hsHKR
OTD in 2012, sister Voyager 1 made her final transition from the region dominated by our Sun's solar wind into the region dominated by the other stars' cumulative winds: 'interstellar space.' For the first time, we were measuring particles mainly from other stars.
The measurements are from the LECP instrument, and the oscillations in late July and August show the buffeting nature of the boundary as it billows out from the Sun and then is pushed back by interstellar pressure, with the boundary moving back and forth over Voyager 1 several times. The August 25, 2012 transition occurred at a distance of 16H:51M light-time from the Sun, or about 121.6 AU.
Voyager 2 encountered this boundary in 2018 from early November to early December, but the boundary was smoother and closer in: from 16H30M to 16H32M, or 119.0 to 119.3 AU. Both crossings occurred during solar sunspot cycle 24, with the V2 crossing possibly occurring at a quieter time.
The historic first Earthrise photo from the Moon was received 60 years ago today. It was shot on film, developed onboard the Lunar Orbiter 1 spacecraft, scanned, transmitted home...and then meticulously restored decades later.
https://t.co/0Vinhsc02u
At a meeting of the International Astronomical Union 20 years ago today, astronomers vote on a definition of a "planet." The new criteria:
🌘 Must orbit its host star
🌓 Must be mostly round
🌒 Must be massive enough to clear away other objects of similar size in its orbit
Pluto fails on the third condition and becomes a dwarf planet.