#Uranus

Astronomy Picture of the Dayapod@mastodon.bot
2026-02-24

APOD from 2026-02-24

#Planet Parade over Sydney Opera House

This week, just after sunset, #Mercury, #Venus, #Saturn, and #Jupiter are visible to the naked eye in a line from the horizon. #Uranus and #Neptune can be seen with a #telescope. Best viewed this weekend globally along the ecliptic plane.

HD image at apod.nasa.gov/apod/ap260224.ht #astronomy #planets #earth

Planet Parade over Sydney Opera House
Taran Rampersadknowprose
2026-02-24

I honestly think some scientists just study for headline giggles. But it's pretty cool.

Those auroras around Uranus.

gizmodo.com/webb-just-spent-17

Astrology Healsastrologyheals
2026-02-23

Monday, February 23rd, 2026

Today the 🌒 continues in , bringing ♉

a focus to physical needs. 🍲

As the Moon joins ,

we could see some

unexpected developments. ⚡

Make way for ➡️

new information 📰

as the Moon shifts into ! 🧐

Details in this video youtu.be/hpiTPN2HW0c

KUVO Playlistkuvo_playlist
2026-02-22

2:55pm Uranus by Steve Berrios & Son Bachéche from First World

2026-02-22

The Webb telescope watched Uranus for 17hrs to create this video of a complete rotation and massive aurora!

esa.int/ESA_Multimedia/Videos/

#space #science #uranus #WebbTelescope

Kuuke's Sterrenbeeldenkuuke@mastodon.nl
2026-02-22

Webb onthult verborgen lagen van de bovenste atmosfeer van Uranus
Astronomen hebben voor het eerst de verticale structuur van de ionosfeer van Uranus in kaart gebracht. Daarbij ontdekten ze onverwachte
#ijsreus #ionosfeer #planeet #temperatuur #uranus #WebbSpaceTelescope #zonnestelsel
kuuke.nl/webb-onthult-verborge

De bovenste atmosfeer van Uranus
Where are we now?wawn
2026-02-20

2026-02-20 12:00:00 UTC (Delta: 2026-02-13)

URANUS
- Distance (km): 2,921,655,418.80 km (+17,834,269.61 km)
- Distance (AU): 19.53 (+0.12)
- Light travel time: 2 h 42 min 25.59 s (+59.49 s)
- Orbital speed: 6.71 km/s (+0.00 km/s)

Image: Alien aurorae spotted on Uranus by Hubble
Credit: NASA Goddard

This is a composite image of Uranus by Voyager 2 and two different observations made by Hubble — one for the ring and one for the auroras.

Ever since Voyager 2 beamed home spectacular images of the planets in the 1980s, planet-lovers have been hooked on auroras on other planets. Auroras are caused by streams of charged particles like electrons that come from various origins such as solar winds, the planetary ionosphere, and moon volcanism. They become caught in powerful magnetic fields and are channeled into the upper atmosphere, where their interactions with gas particles, such as oxygen or nitrogen, set off spectacular bursts of light.

The auroras on Jupiter and Saturn are well-studied, but not much is known about the auroras of the giant ice planet Uranus. In 2011, the NASA/ESA Hubble Space Telescope became the first Earth-based telescope to snap an image of the auroras on Uranus. In 2012 and 2014 a team led by an astronomer from Paris Observatory took a second look at the auroras using the ultraviolet capabilities of the Space Telescope Imaging Spectrograph (STIS) installed on Hubble.

They tracked the interplanetary shocks caused by two powerful bursts of solar wind traveling from the sun to Uranus, then used Hubble to capture their effect on Uranus’ auroras — and found themselves observing the most intense auroras ever seen on the planet. By watching the auroras over time, they collected the first direct evidence that these powerful shimmering regions rotate with t...
2026-02-20

Uranus collage (January 2025, annotated) 🛰️🪐

#Uranus

▶️ 1 new picture from ESA commons.wikimedia.org/wiki/Fil

Uranus_collage_(January_2025,_annotated)_ESA518025.jpg
Daniel Fischercosmos4u@scicomm.xyz
2026-02-20

JWST Discovers the Vertical Structure of #Uranus' Ionosphere: agupubs.onlinelibrary.wiley.co -> Webb maps the mysterious upper atmosphere of Uranus: esawebb.org/news/weic2602/ - Webb provides the first vertical view of the planet’s ionosphere, revealing auroras shaped by its tilted magnetic field.

For the first time, an international team of astronomers have mapped the vertical structure of Uranus’s upper atmosphere, uncovering how temperature and charged particles vary with height across the planet. Using Webb’s NIRSpec instrument, the team detected the faint glow from molecules high above the clouds. These unique data provide the most detailed portrait yet of where the planet’s auroras form, how they are influenced by its unusually tilted magnetic field, and how Uranus’s atmosphere has continued to cool over the past three decades. The results offer a new window into how ice-giant planets distribute energy in their upper layers.
QuestingFatherquestingfather
2026-02-17

Stopover at Oshpak's House on Titania (Uranus' third moon) to pay an Aegis Core fine. I even tended the bar and saw a shaken traveler after a guard scan. Titania's easy to miss, so we doubled back. Catch the next Sol Tour stream Wednesday at 6 PM CT.

Astrology Healsastrologyheals
2026-02-16

Monday, February 16th, 2026

Tomorrow's 🌑 in

invites us to:

✨ access new ideas 💡
✨ align with a vision for the future 💫
✨ work in communities to make it happen 🌎

is in , emphasizing

a need to uphold our values 📜

through clearsighted vision. 👀

More about Uranus, and the Moon's

conjunction to ...

Details in this video youtu.be/V4cn-3_lzMM

2026-02-15

An exoplanetary system about 116 light-years from Earth could flip the script on how #planets form.

Four planets orbit LHS 1903 — a red dwarf #star, the most common type of star in the #universe — and are arranged in a peculiar sequence.

The innermost #planet is rocky, while the next two are gaseous, and then, unexpectedly, the outermost planet is also rocky.

This arrangement contradicts a pattern commonly seen across the galaxy and in our own solar system, where the rocky planets (#Mercury, #Venus, #Earth and #Mars) orbit closer to the sun and the gaseous ones (#Jupiter, #Saturn, #Uranus and #Neptune) are farther away.

Astronomers suspect this common pattern arises because planets form within a disk of gas and dust around a young star, where temperatures are much higher close to the celestial body.

In these inner regions, volatile compounds such as water and carbon dioxide are vaporized while only materials that can withstand extreme heat — such as iron and rock-forming minerals — can clump together into solid grains. The planets that form there are therefore primarily rocky.

A discovery of a planet breaking this pattern is telling about anomalies in the common formation process.

#exoplanets #astronomy
ksl.com/article/51447598/astro

QuestingFatherquestingfather
2026-02-15

A serene glimpse of the ice giant Uranus from our travels. The calm before the next journey into the black.

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