Juno: Inside The Spacecraft

Juno: Inside the Spacecraft

Our Juno spacecraft was carefully designed to meet the tough challenges in flying a mission to Jupiter: weak sunlight, extreme temperatures and deadly radiation. Lets take a closer look at Juno:

It Rotates!

Roughly the size of an NBA basketball court, Juno is a spinning spacecraft. Cartwheeling through space makes the spacecraft’s pointing extremely stable and easy to control. While in orbit at Jupiter, the spinning spacecraft sweeps the fields of view of its instruments through space once for each rotation. At three rotations per minute, the instruments’ fields of view sweep across Jupiter about 400 times in the two hours it takes to fly from pole to pole.

It Uses the Power of the Sun

Jupiter’s orbit is five times farther from the sun than Earth’s, so the giant planet receives 25 times less sunlight than Earth. Juno will be the first solar-powered spacecraft we’ve designed to operate at such a great distance from the sun. Because of this, the surface area of the solar panels required to generate adequate power is quite large.

Three solar panels extend outward from Juno’s hexagonal body, giving the overall spacecraft a span of about 66 feet. Juno benefits from advances in solar cell design with modern cells that are 50% more efficient and radiation tolerant than silicon cells available for space missions 20 years ago. Luckily, the mission’s power needs are modest, with science instruments requiring full power for only about six out of each 11-day orbit.

It Has a Protective Radiation Vault

Juno will avoid Jupiter’s highest radiation regions by approaching over the north, dropping to an altitude below the planet’s radiation belts, and then exiting over the south. To protect sensitive spacecraft electronics, Juno will carry the first radiation shielded electronics vault, a critical feature for enabling sustained exploration in such a heavy radiation environment.

Juno Science Payload:

Gravity Science and Magnetometers – Will study Jupiter’s deep structure by mapping the planet’s gravity field and magnetic field.

Microwave Radiometer – Will probe Jupiter’s deep atmosphere and measure how much water (and hence oxygen) is there.

JEDI, JADE and Waves – These instruments will work to sample electric fields, plasma waves and particles around Jupiter to determine how the magnetic field is connected to the atmosphere, and especially the auroras (northern and southern lights).

JADE and JEDI

Waves

UVS and JIRAM – Using ultraviolet and infrared cameras, these instruments will take images of the atmosphere and auroras, including chemical fingerprints of the gases present.

UVS

JIRAM

JunoCam – Take spectacular close-up, color images.

Follow our Juno mission on the web, Facebook, Twitter, YouTube and Tumblr.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

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7 years ago

SpaceX Dragon breathes Astronomical Amounts of Science to Space Station

SpaceX is helping the crew members aboard the International Space Station get down and nerdy as they launch their Dragon cargo spacecraft into orbit for the 13th commercial resupply mission, targeted for Dec. 15 from our Kennedy Space Center in Florida.

This super science-heavy flight will deliver experiments and equipment that will study phenomena on the Sun, materials in microgravity, space junk and more.

Here are some highlights of research that will be delivered to the station:

ZBLAN Fiber Optics Tested in Space!

The Optical Fiber Production in Microgravity (Made in Space Fiber Optics) experiment demonstrates the benefits of manufacturing fiber optic filaments in a microgravity environment. This investigation will attempt to pull fiber optic wire from ZBLAN, a heavy metal fluoride glass commonly used to make fiber optic glass.

When ZBLAN is solidified on Earth, its atomic structure tends to form into crystals. Research indicates that ZBLAN fiber pulled in microgravity may not crystalize as much, giving it better optical qualities than the silica used in most fiber optic wire.

Total and Spectral Solar Irradiance Sensor is Totally Teaching us About Earth’s Climate

The Total and Spectral Solar Irradiance Sensor, or TSIS, monitors both total solar irradiance and solar spectral irradiance, measurements that represent one of the longest space-observed climate records. Solar irradiance is the output of light energy from the entire disk of the Sun, measured at the Earth. This means looking at the Sun in ways very similar to how we observe stars rather than as an image with details that our eye can resolve.

Understanding the variability and magnitude of solar irradiance is essential to understanding Earth’s climate.

Sensor Monitors Space Station Environment for Space Junk

The Space Debris Sensor (SDS) will directly measure the orbital debris environment around the space station for two to three years.

Above, see documentation of a Micro Meteor Orbital Debris strike on one of the window’s within the space station’s Cupola.

Research from this investigation could help lower the risk to human life and critical hardware by orbital debris.

Self-Assembling and Self-Replicating Materials in Space!

Future space exploration may utilize self-assembly and self-replication to make materials and devices that can repair themselves on long duration missions.

The Advanced Colloids Experiment- Temperature-7 (ACE-T-7) investigation involves the design and assembly of 3D structures from small particles suspended in a fluid medium.

Melting Plastics in Microgravity

The Transparent Alloys project seeks to improve the understanding of the melting and solidification processes in plastics in microgravity. Five investigations will be conducted as a part of the Transparent Alloys project.

These European Space Agency (ESA) investigations will allow researchers to study this phenomena in the microgravity environment, where natural convection will not impact the results.

Studying Slime (or…Algae, at Least) on the Space Station

Arthrospira B, an ESA investigation, will examine the form, structure and physiology of the Arthrospira sp. algae in order to determine the reliability of the organism for future spacecraft biological life support systems.

The development of these kinds of regenerative life support systems for spaceflight could also be applied to remote locations on Earth where sustainability of materials is important.

Follow @ISS_Research on Twitter for more space science and watch the launch live on Dec. 15 at 10:36 a.m. EDT HERE!

For a regular dose of space-nerdy-goodness, follow us on Tumblr: https://nasa.tumblr.com/.

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9 years ago

What’s Up for December?

View Mars right now, and prepare for 2016, the best Mars viewing year since 2005! Last month early risers watched small, reddish Mars dance with brighter Jupiter and Venus just before sunrise.

This month Mars rises earlier-by about 2 a.m. local time. Its reddish color is unmistakable, even without a telescope. It’s easy to see below the Moon and Jupiter on December 4. You won’t see many features this month, because the planet is almost 10 times smaller than nearby Jupiter appears and 350 times smaller than the Moon appears to us on Earth.

You should also be able to see Mars’ north polar region this month, because it’s currently tilted towards Earth.

You’ll be amazed at the changes you’ll see during 2016. January through December are all prime Mars observing months. Between January and May next year, Mars triples in apparent diameter as its orbit around the sun brings it closer to Earth. You’ll even be able to see the areas on Mars where NASA’s Mars landers are located.

By October, Mars shrinks in apparent size to less than half its May diameter as it speeds away from Earth. Mars shrinks even further from October through December, returning to the same size we saw in January 2016 by year’s end.

So put Mars viewing on your calendar for 2016. You won’t see Mars this size again until 2018, when Mars will put on an even better show.