NASA readies its most explosive rocket for round the moon flight

Artemis II mission could launch on February 6 sending astronauts on 685000 mile journey.

Nasa is preparing roll out its most explosive rocket before mission to send astronauts around the moon and back again for first time in over 50 years.

The Artemis II mission scheduled to launch from Kennedy Space Center in Florida as early as 6 February taking its crew on 685000 mile round trip that will end about 10 days later with splashdown in Pacific Ocean.

The flight will mark only second test of Nasa Space Launch System SLS rocket and first with crew onboard.

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The four astronauts will live and work in Orion capsule testing life support and communication system and practising docking manoeuvre.

Its a big deal said David Parker ex head of UK Space Agency and visiting professor at University of Southhampton.

“It is a move towards what we in space world always dreamed of the sustained human and robotic exploration of moon and one day on to Mars”

Some paint the return to moon as second space race with USA contesting agains Chine. which hopes to put own boot on moon by 2030.

I shall be damned if chinese beat Nasa or beat America back to moon. Sean Duff Nasa ex acting administrator said in September.

We are going to win.

The flight will mark only second test of Nasa Space Launch System SLS rocket and first with crew onboard.

The four astronauts will live and work in Orion capsule testing life support and communication system and practising docking manoeuvres.

Jared Isaacman the billionaire private astronaut sworn in as Nasa administrator in December said on Thursday the mission was probable one of most important human spaceflight mission in last half century.

It will be second time in space for three Nasa astronauts. Reid Wiseman Victor Glover and Christina Koch and first for Jeremy Hansen a Canadian astronaut Koch will become first lady and Glover the first person of colour to travel beyond low Earth orbit.

The astronauts will not land on moon or enter lunar orbit but will be first to travel around moon since Apollo 17 in 1972.

The SLS rocket and Orion capsule almost 100 meters tall with rocket carrying over enough liquid propellant to fill olympic sized swimming pool.

When burned through the rocket engines it produces enough thrust to fly to moon at speed of up to 24500 mph.

Over 50 year after humans went to moon it is time to get excited again. Every rocket launch is nail biter Parker said.

We are putting astronauts on a rocket and flown only once before so of course it is a nail biter.

For all Nasa preparations and astronaut expensive training the mission could throw some stunning wonders.

This is test flight and there are things that are going to be unexpected said Jeff Radigan Artemis II lead flight director.

An ultimate push from Orion Europe service module will send the crew to moon.

The astronauts will travel over 230000 miles from Earth passing around far side of moon before looping back in mega figure of eight trajectory.

During the travel the crew will practise emergency procedures and test Orion radiation shelter designed to save them from harmful solar flares.

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Nasa crawler transporter 2 and huge tracked vehicle will start lugging the 5000 tonne rocket and spacecraft from vehicle assembly building to launchpad.

The four mile journey can take up to 12 hours.

NASA will work through a preflight checklist.

It all goes to plan engineers will move on to wet dress rehearsal loading rocket with over 700,000 gallons of propellant conducting a trial countdown and demonstrating that they can remove propellant safely.

Any mega problems would require rocket to be rolled back to vehicle assembly building for repairs.

In latest days, technicians have been working on bent cable in rocket flight termination system a faulty valve used to pressurise the Orion capsule and leaks in instruments that pumps oxygen into spacecraft.

The complete process must go smoothly for mission to launch on 6 February.

If technical problems or bad weather involve Nasa identified 14 other dates to launch before mid April.

After liftoff the crew will loop twice around Earth. Before moving to moon the Orion capsule will separate from rocket upper stage.

The astronauts will fly the spacecraft manually using cameras and view outside the window to approach and retreat the jettisoned stage.

This will give Nasa sense of how Orion handles for future Artemis missions where crew will dock and undock in lunar orbit.

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Web Telescope Spots “Impossible” Atmosphere Around Ancient Super Earth

JWST observations of the ultra hot super Earth exoplanet TOI-561 provide the evidence to date for atmosphere surrounding rocky planet beyond our solar system.

A team of astronomer led by Carnegie researchers has uncovered the clearest evidence so far a rocky planet outside our  Solar System possesses an atmosphere.

The findings reported in The Astrophysical Journal Letters are based on observations from NASA James Webb Space Telescope JWST.

The data indicates the presence of atmosphere on unlikely world an ancient extreme hot super Earth that is thought to be covered by global ocean of molten rock.

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The planet called TOI-561 b is twice as massive as Earth but is otherwise very different from our planet.

Its extreme conditions are driven by its tight orbit around its star.

The star itself is smaller and cooler than the Sun, TOI-561 b circles it one fortieth the distance between Sun and Mercury.

This close orbit the planet completed a full year in only 10.56 hours and one hemisphere is exposed to starlight.

Astronomers would have predicted that planet like this is too small and hot to retain its own atmosphere for long after formation explained Carnegie Science Postdoctoral Fellow Nicole Wallack the paper second author.

Our observations suggest it is surrounded by relative thick blanket of gas spending conventional wisdom about ultra short period planets.

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JWST observations

These are first results from JWST General Observers Program 3860 which involved observing the system continuously for over 37 hours while TOI-561 b completed almost for full orbits of the star.

The team is analyzing the full data set to map the temperature all the method around the planet and narrow down  the composition of atmosphere.

Teske and Wallack leadership on this JWST paper present a tradition of Carnegie Science excellence dating back to mission conception three decades before and extending through first four cycles of  time allocation on revolutionary space telescope.

JWST finished calibrations and start collecting data for astronomical research programs, Teske, Wallack and other Carnegie Earth and Planets Laboratory and Observatories  affiliated scientists have led over dozen JWST teams and announced groundbreaking results about exoplanet atmospheres  galaxy formation.

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These JWST powered breakthroughs tap directly into our long standing strength in how exoplanet characters are shaped by planetary evolution and dynamics.

There are more results on horizon and we are poised for new wave of Carnegie led JWST science in year ahead.

Challenging Planetary Expectations

In our own solar system planets that are small and intense heated were unable to keep the original gaseous envelops they acquired in their histories.

TOI-561 b appears to have held on its atmosphere even though it orbits a star that is older than the sun.

This lingering atmosphere may account for other puzzle the planets surprisingly low density.

TOI-561 b is lighter than scientist would expect based on size alone and presence of atmosphere could help explain why.

It is not what we call a super puff or cotton candy planet but it is less dense than you would expect if it had earth like composition.

In designing the observing program the team considered that planet low density could be explained by relative small iron core and mantle made of rock is less dense than rocks that comprise Earth interior.

Teske points that this could make sense TOI-561 b is distinct among ultra short period planets in that it orbits a old twice as old as Sun iron poor star in a region of Milky Way famous as thick disk.

It must have shaped in different chemical environment from planets in our own Solar System.

This mean that composition could be representative of planets that formed when universe was relatively young.

Searching for Atmosphere

In deciding to study TOI-561 b the research team suspect that it might be surrounded by thick atmosphere that makes it look larger and thus less dense.

To test existence of TOI-561 b atmosphere the astronomer used JWSY Near Infrared Spectrograph NIRSpec instrument to measure the planet dayside temperature based on brightness in near infrared.

The technique which consist of measuring the decrease in brightness of star planet system as the planet moves behind the star is similar to search for atmospheres in the TRAPPIST-1 system and other rocky worlds.

The ALMA Array is completed with 145 New Low Noise Amplifiers

For decades scientists have observed the cosmos with radio antennas to visualize the dark distant regions of the Universe.

This consist of the gas and dust of the interstellar medium ISM planet forming disks and objects that cannot be observed in visible light.

In this field the Atacama Large Millimeter/Submillimeter Array ALMA in Chile stands out as one of world powerful radio telescopes.

Using its 66 parabolic antennas, ALMA observes the millimeter and submillimeter radiation emitted by  cold molecular clouds from which new stars are born.

Each antenna is equipped with high frequency receivers for ten wavelength ranges 35-50 GHZ and 787-950 GHZ known as Band 1.

The ALMA Array is completed with 145 New Low Noise Amplifiers

Thanks to Fraunhofer Institute for Applied Solid State Physics IAF and the Max Planck Institute for Radio Astronomy MPIFR, ALMA has received upgrade with addition of 145 new low noise amplifiers LNAs.

These amplifiers are part of facilities Band 2 coverage ranging from 67 to 116 GHz on the electromagnetic spectrum.

This coverage will allow researchers to study and gain better understanding of Universe.

They hope to gain new insights into cold interstellar medium the dust, gas radiation and magnetic fields from which stars are born.

Scientist will be able to study planet forming disk in better detail.

But certainly not least they will be able to study complex organic molecules COM in nearby galaxies which considered precursors to building blocks of life DNA, RNA.

These studies will allow astronomers and cosmologists to witness how stars and planetary systems form and evolve and how presence of organic molecules can lead to emergence of life.

Each LNA consist of a series of monolithic microwave integrated circuits MMICs developed by Frauhofer IAF using the semiconducting material indium gallium arsenide INGAAS.

The ALMA Array is completed with 145 New Low Noise Amplifiers

MMICs are based on metamorphic high electron mobility transistor mHEMT technologt a method for creating advance transistors that are flexible and allow for performance in high frequency receivers.

The addition of LNAs equipped with these circuits will amplify low noise signals and minimize background noisce increasing the sensitivity of ALMAs receivers.

Frauhofer IAF and MPIFR were commissioned by the European Southern Observatory ESO to provide amplifiers.

Frauhofer IAF was responsible for designing, testing and manufacturing the MMICs at room temperature, MPIFR was task with assembling and qualifying the LNA modules, then testing them in cryogenic conditions.

This is wonderful recognition of our fantastic collaboration with Fraunhofer IAF which shows that amplifiers are not only made in Germany but best in world said Prof Dr. Michael Kramer executive director at MPIFR.

Dr Fabian Thome head of subproject at Frauhofer IAF explained in IAF press release.

The performance of receivers depend on the performance of the first high frequency amplifiers installed in them.

Our technology is characterized by an average noise temperature of 22 K which is unmatched worldwide.

The ALMA Array is completed with 145 New Low Noise Amplifiers

New LNA signals can be amplified more than 300 fold in first step.

This enables the ALMA receivers to measure millimeter and submillimeter radiation from depths of universe much more precisely and obtain better data.

We are proud that our LNA technology is helping us to better understand the origin of stars and entire galaxies.

James Webb Telescope spies a monstrous molecular cloud shrouded in mystery Space Image of the Week

In this James Webb telescope photo the mega molecular cloud near our galaxy center appears as canvas of pink and purple clouds set against shadow backdrop.

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Stars shape in molecular clouds molecular clouds regions that are cold, dense, rich in molecules and filled with dust.

One huge cloud responsible for forming half of stars in Milky Way central region is Sagittarius B2 molecular cloud located in few hundred light years from our central supermassive black hole.

Boasting a mega mass between 3 million and 10 millions time that of sun and stretching 150 light year across.

It is one mega molecular clouds in galaxy.

It lies almost 26000 light years from Earth in constellation Sagittarius.

It is chemically rich.

Several complex molecules discovered.

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