Anonymous ID: 71488d July 15, 2024, 6:47 a.m. No.21209590   🗄️.is 🔗kun   >>9607

NASA Astronomy Picture of the Day

July 15, 2025

 

The Tadpole Galaxy from Hubble

 

Why does this galaxy have such a long tail? In this stunning vista, based on image data from the Hubble Legacy Archive, distant galaxies form a dramatic backdrop for disrupted spiral galaxy Arp 188, the Tadpole Galaxy. The cosmic tadpole is a mere 420 million light-years distant toward the northern constellation of the Dragon (Draco). Its eye-catching tail is about 280 thousand light-years long and features massive, bright blue star clusters. One story goes that a more compact intruder galaxy crossed in front of Arp 188 - from right to left in this view - and was slung around behind the Tadpole by their gravitational attraction. During the close encounter, tidal forces drew out the spiral galaxy's stars, gas, and dust forming the spectacular tail. The intruder galaxy itself, estimated to lie about 300 thousand light-years behind the Tadpole, can be seen through foreground spiral arms at the upper right. Following its terrestrial namesake, the Tadpole Galaxy will likely lose its tail as it grows older, the tail's star clusters forming smaller satellites of the large spiral galaxy.

 

https://apod.nasa.gov/apod/astropix.html?

Anonymous ID: 71488d July 15, 2024, 7:30 a.m. No.21209833   🗄️.is 🔗kun

Evidence of water found in atmosphere of mysterious 'metal god of war' exoplanet

July 15, 2024

 

Astronomers may have discovered the presence of water in the atmosphere of a blisteringly hot planet that is also one of the most "metal" worlds ever spotted.

The planet's formation remains a mystery, one that could be solved by the discovery.

The extra-solar planet, or "exoplanet," in question is HD 149026 b, which is also known as "Smertrios," meaning the "Purveyor" or "The Provider," worshiped as the god of war in the Gaelic tradition.

Smertrios orbits a yellow subgiant star called HD 149026, located around 247 light-years from Earth.

 

The planet is around 4 million miles from its parent star, completing an orbit in under three Earth days.

With a width of about three-quarters that of Jupiter, Smertrios is classed as a "hot Saturn," a class of planets taking its name from the solar system's smaller gas giant.

The proximity of Smertrios to its star means that it is tidally locked with a permanent dayside that always faces its host star, where temperatures soar as high as 2,600 degrees Fahrenheit (1,420 degrees Celsius).

It's relatively cooler nightside always faces out into space. But the density and composition of Smertrios, discovered in 2005 as it crossed or "transited" the face of its star, are what really make it really strange.

 

"A hot Saturn is a type of exoplanet called a 'hot gas giant.' Hot gas giants are exoplanets that have sizes similar to Jupiter or Saturn but orbiting their host stars in extremely close distances. Typically, they have an orbital period of less than ten days, meaning that one year on those planets could be less than a week!" Sayyed Ali Rafi, part of the team behind the discovery and an astronomy researcher at the University of Tokyo, told Space.com. "This planet is of particular interest because it is one of the most metal-rich and densest gas giants that we know of so far."

When astronomers like Ali Rafi refer to "metals," they are elements that are heavier than hydrogen and helium.

When the James Webb Space Telescope (JWST ) looked at Smertrios in 2023, the powerful space telescope found that the planet's metallicity, its fraction of metals to hydrogen, is much higher than most hot Saturns and larger hot Jupiters.

 

This ratio is also much greater for Smertrios than it is for solar system giants Jupiter and Saturn.

Metals are normally considered to be conversely proportional to mass in gas giants. That means the bigger a gas giant gets, the less metals it should have. Smertrios defies this trend.

The planet was also found to have an anomalously large solid core, which is why its density is so high.

 

"The composition of the planet seems not to be compatible with current formation scenarios that we have for hot gas giants, and it is still a mystery to this day," said Ali Rafi.

"This signifies the importance of observing the planet’s atmosphere as it could help reveal the planet's formation history through its atmospheric properties such as its metallicity and carbon to oxygen ratio."

To investigate the strange atmosphere of Smertrios and hopefully discover why the planet is so "metal," Ali Rafi and colleagues turned to the CARMENES spectrograph, an instrument at the Calar Alto Observatory in Spain.

Elements and chemical molecules absorb and emit light at characteristic wavelengths.

 

When a planet like Smertrios transits the face of its star, the elements in its atmosphere leave "fingerprints" in the filtered starlight. CARMENES can read these fingerprints and tell astronomers what that atmosphere is made of.

The investigation of Smertrios with CARMENES revealed the fingerprints of water vapor. This can help to better constrain the abundance of other elements in the planet's atmosphere.

Ali Rafi explained that assuming elemental oxygen is more abundant than elemental carbon in the atmosphere of hot gas giants such as Smertrios means water and carbon monoxide are two of the most abundant "tracer" species that can explain the nature of that atmosphere.

 

"Hence, if we can constrain the abundance of both molecules, we are able to constrain the atmospheric carbon to oxygen ratio, which is very important because it could act as a kind of tracer characteristic to the formation and evolution history of gas giant planets like HD 149026 b," Ali Rafi added. "Finding water in the atmosphere is the first step to such characterization, hence its importance."

However, this wasn't all the team discovered about Smertrios. The hot Saturn planet delivered quite a surprise for the researchers.

 

cont.

 

https://www.space.com/exoplanet-water-atmosphere-metal-smertrios