Universe Today

April 2, 2015December 23, 2015 by Matt Williams

The Orion’s Heat Shield Gets a Scorching on Re-entry

Larry Gagliano, Orion project manager at NASA's Marshall Space Flight Center, photographed in front of the spaceship's heat shield. Credit: Lee Roop

Yes, she’s a little worse for wear, isn’t she? But then again, that’s what atmospheric re-entry and 2200 °Celsius (4000 °Fahrenheit) worth of heat will do to you! Such was the state of the heat shield that protected NASA’s Orion Spaceship after it re-entered the atmosphere on Dec. 5th, 2014. Having successfully protected the craft during it’s test flight, the shield was removed and transported to the Marshall Space Flight Center in Huntsville, Alabama, where it arrived on March. 9th.

Since that time, a steady stream of NASA employees have been coming by the facility to get a look at it while engineers collect data and work to repair it. In addition to being part of a mission that took human-rated equipment farther out into space than anything since the Apollo missions, the heat shield is also living proof that NASA is restoring indigenous space capability to the US.

First unveiled by NASA in May of 2011, the Orion Multi-Purpose Crew Vehicle (MPCV) was intrinsic to the Obama administration’s plan to send astronauts to a nearby asteroid by 2025 and going to Mars by the mid-2030’s. In addition to facilitating these long-range missions, the Orion spacecraft would also handle some of the routine tasks of spaceflight, such as providing a means of delivering and retrieving crew and supplies from the ISS.

NASA Orion spacecraft blasts off atop 1st Space Launch System rocket in 2017 - attached to European provided service module – on an enhanced m mission to Deep Space where an asteroid could be relocated as early as 2021. Credit: NASA — *Artist’s concept of the Orion spacecraft being sent into orbit atop the first Space Launch System (SLS) rocket in 2017. Credit: NASA*

The uncrewed test flight that took place on December 5, 2014, known as Exploration Flight Test 1 (EFT-1), was intended to test various Orion systems, including separation events, avionics, heat shielding, parachutes, and recovery operations prior to its debut launch aboard the Space Launch System,

This design of this mission corresponded to the Apollo 4 mission of 1967, which demonstrated the effectiveness of the Apollo flight control systems and the heat shields ability to withstand re-entry conditions, as part of the spacecraft’s return from lunar missions.

After being retrieved, the heat shield was transported by land to the Marshall Space Flight Center, where it was offloaded and transferred to a large support structure so engineers could perform studies on it for the next three months.

This will consist of collecting samples from the shield to measure their char layers and degree of erosion and ablation, as well as extracting the various instruments embedded in the heat shield to assess their performance during re-entry.

The heat shield arrived March 9 at Marshall, where experts from the Center and NASA’s Ames Research Center will extract samples of the ablative material, or Avcoat. Image Credit: NASA/MSFC/Emmett Given — *The heat shield arriving at Marshall on March 9th, where experts from the Center and NASA’s Ames Research Center. Credit: NASA/MSFC/Emmett Given*

After the analysis is complete, technicians will load the shield into the 7-axis milling machine and machining center, where it will be grind down to remove the remaining material covering. Known as Avcoat, this heat-retardant substance is similar to what the Apollo missions used, with the exception of toxic materials like asbestos.

This material is used to fill the 320,000 honeycomb-like cells that make up the outer layer of the shield. When heated, the material burns away (aka. ablates) in order to prevent heat being transferred into the crew module. This shield is placed over the craft’s titanium skeleton and carbon-fiber skin, providing both protection and insulation for the interior.

Once all the Avcoat is removed and only the skeletal frame remains, it will be shipped to the Langley Research Center in Hampton, Virginia, for more tests. Since the Orion was returning from a greater distance in space than anything since Apollo, it experienced far greater heat levels than anything in recent decades, reaching as high as 2200 °C (4000 °F).

During Orion's test flight the heat shield reached temperatures of about 4,000 degrees Fahrenheit. Instrumentation in the heat shield measured the rise of the surface and internal temperatures during re-entry as well as heating levels and pressures. Image Credit: NASA/MSFC/Emmett Given — *Instrumentation in the Orion heat shield (visible here) measured the rise of the surface and internal temperatures during re-entry. Credit: NASA/MSFC/Emmett Given*

Instrumentation in the shield measured the rise of the surface and internal temperatures during re-entry as well as the ablation rate of the shield’s coating. Over the next few months, NASA experts will be pouring over this data to see just how well the Orion shield held up under extreme heat. But so far, the results look positive – with only 20% of the Avcoat burning away on the test-flight re-entry.

In the future, the Orion spacecraft will be launched on Space Launch System on missions that will take it to nearby asteroids and eventually Mars. The first mission to carry astronauts is not expected to take place until 2021 at the earliest.

Further Reading: NASA

April 2, 2015October 10, 2016 by David Dickinson

Adventures in Satspotting: Why Are Different Orbits Needed for Satellites?

Congratulations: perhaps you’re a new space-faring nation, looking to place a shiny new payload around the planet Earth. You’ve assembled the technical know-how, and seek to break the surly bonds and join an exclusive club that thus far, only contains 14 nations capable of indigenous spaceflight. Now for the big question: which orbit should you choose?

Welcome to the wonderful world of orbital mechanics. Sure, satellites in orbit have to follow Newton’s laws of motion, as they perpetually ‘fall’ around the Earth without hitting it. But it’ll cost you in fuel expended and technical complexity to achieve different types of orbits. Different types of orbits can, however, be used to accomplish different goals.

The first artificial moon to be placed in low-Earth orbit was Sputnik 1 launched on October 4^th, 1957. But even before the dawn of the Space Age, visionaries such as futurist and science fiction author Arthur C. Clarke realized the value of placing a satellite in a geosynchronous orbit about 35,786 kilometres above the Earth’s surface. Placing a satellite in such an orbit keeps it in ‘lockstep’ with the Earth rotating below it once every twenty four hours.

Here are some of the more common orbits targeted by modern satellites and their uses:

Low-Earth Orbit (LEO): Placing a satellite 700 km above the surface of the Earth moving 27,500 km per hour will cause it to orbit the Earth once every 90 minutes. The International Space Station is in just such an orbit. Satellites in LEO are also subject to atmospheric drag, and must be boosted periodically. Launching from the equator of the Earth gives you an initial free maximum 1,670 km/per hour boost into orbit eastward. Incidentally, the high 52 degree inclination orbit of the ISS is a compromise that assures that it is reachable from various launch sites worldwide.

Low Earth orbit is also becoming crowded with space junk, and incidents such as the successful 2007 anti-satellite missile test by China, and the 2009 collision of Iridium 33 and the defunct Kosmos-2251 satellite both showered low Earth orbit with thousands of extra pieces of debris and didn’t help the situation much. There have been calls to make reentry technology standard on future satellites, and this will become paramount with the advent of flocks of nano and CubeSats in LEO.

Sun-Synchronous Orbit: This is a highly inclined retrograde orbit that assures that the illumination angle of the Earth below is consistent on multiple passes. Though it takes a fair amount of energy to reach a Sun-synchronous orbit—plus a complex deployment maneuver known as a ‘dog leg’—this type of orbit is desirable for Earth observing missions. It’s also a favorite for spy satellites, and you’ll notice that many nations aiming to put up their first satellites will use the stated goal of ‘Earth observation’ to field spy satellites of their own.

Molyina orbit: A highly inclined elliptical orbit designed by the Russians, a Molyina orbit takes 12 hours to complete, placing the satellite over one hemisphere for 2/3rds of its orbit and returning it back over the same geographical point once every 24 hours.

A semi-synchronous orbit: A 12-hour elliptical orbit similar to a Molyina orbit, a semi-synchronous orbit is favored by Global Positioning Satellites.

Geosynchronous orbit: The aforementioned point 35,786 km above the Earth’s surface where a satellite stays fixed over a particular longitude.

Geostationary orbit: Place a GEO satellite in orbit with a zero degree orbit, and it is considered Geostationary. Also sometimes referred to as a Clarke orbit, this location is extremely stable, and satellites placed there may remain in orbit for millions of years.

In 2012, the EchoStar XVI satellite was launched headed to GEO with the time capsule disk The Last Pictures for just that reason. It is quite possible that millions of years from now, GEO sats might be the primary artifacts remaining from the early 20th/21st century civilization.

Lagrange point orbits: 18th century mathematician Joseph-Louis Lagrange made the observation that several stable points exist in any three body system. Dubbed Lagrange points, these locales serve as great stable positions to place observatories. The Solar Heliospheric Observatory (SOHO) sits at the L1 point to afford it a continuous view of the Sun; the James Webb Space Telescope is bound in 2018 for the L2 point beyond the Moon. To stay on station near a LaGrange point, a satellite must enter a Lissajous or Halo orbit around the imaginary Lagrange point in space.

All of these orbits have pros and cons. For example, atmospheric drag isn’t an issue in geosynchronous orbit, though it takes several boosts and transfer orbit maneuvers to attain. And as with any plan, complexity also adds more chances for things to fail, stranding a satellite in the wrong orbit. Russia’s Phobos-Grunt mission suffered just such a fate after launch in 2011 when its Fregat upper stage failed to operate properly, stranding the interplanetary spacecraft in Earth orbit. Phobos-Grunt crashed back to Earth over the Southern Pacific on January 15^th, 2012.

Space is a tough business, and it’s imperative to place things in the right orbit!

-Looking to hunt for satellites from your backyard? A great online resource to start with in Heavens-Above.

April 1, 2015December 23, 2015 by Ken Kremer

OSIRIS-REx Asteroid Sampler Enters Final Assembly

Artist concept of OSIRIS-REx, the first U.S. mission to return samples from an asteroid to Earth. Credit: NASA/Goddard

OSIRIS-Rex, NASA’s first ever spacecraft designed to collect and retrieve pristine samples of an asteroid for return to Earth has entered its final assembly phase.

Approximately 17 months from now, OSIRIS-REx is slated to launch in the fall of 2016 and visit asteroid Bennu, a carbon-rich asteroid.

Bennu is a near-Earth asteroid and was selected for the sample return mission because it “could hold clues to the origin of the solar system and host organic molecules that may have seeded life on Earth,” says NASA.

The spacecraft is equipped with a suite of five science instruments to remotely study the 492 meter meter wide asteroid.

Eventually it will gather rocks and soil and bring at least a 60-gram (2.1-ounce) sample back to Earth in 2023 for study by researchers here with all the most sophisticated science instruments available.

The precious sample would land arrive at Utah’s Test and Training Range in a sample return canister similar to the one for the Stardust spacecraft.

The OSIRIS-REx – which stands for Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer – spacecraft passed a critical decision milestone on the road to launch and has been officially authorized by NASA to transition into this next mission phase.

The decision meeting to give the go ahead for final assembly was held at NASA Headquarters in Washington on March 30 and was chaired by NASA’s Science Mission Directorate, led by former astronaut John Grunsfeld who was the lead spacewalker on the final shuttle servicing mission to the Hubble Space Telescope in 2009.

“This is an exciting time for the OSIRIS-REx team,” said Dante Lauretta, principal investigator for OSIRIS-Rex at the University of Arizona, Tucson, in a stetement.

“After almost four years of intense design efforts, we are now proceeding with the start of flight system assembly. I am grateful for the hard work and team effort required to get us to this point.”

In a clean room facility near Denver, Lockheed Martin technicians began assembling a NASA spacecraft that will collect samples of an asteroid for scientific study. Working toward a September 2016 launch, the OSIRIS-REx spacecraft will be the first U.S. mission to return samples from an asteroid back to Earth. Credit: Lockheed Martin

The transition to the next phase known as ATLO (assembly, test and launch operations) is critical for the program because it is when the spacecraft physically comes together, says Lockheed Martin, prime contractor for OSIRIS-REx. Lockheed is building OSIRIS-Rex in their Denver assembly facility.

“ATLO is a turning point in the progress of our mission. After almost four years of intense design efforts, we are now starting flight system assembly and integration of the science instruments,” noted Lauretta.

Over the next six months, technicians will install on the spacecraft structure its many subsystems, including avionics, power, telecomm, mechanisms, thermal systems, and guidance, navigation and control, according to NASA.

“Building a spacecraft that will bring back samples from an asteroid is a unique opportunity,” said Rich Kuhns, OSIRIS-REx program manager at Lockheed Martin Space Systems, in a statement.

“We can feel the momentum to launch building. We’re installing the electronics in the next few weeks and shortly after we’ll power-on the spacecraft for the first time.”

OSIRIS-REx is scheduled for launch in September 2016 from Cape Canaveral Air Force Station in Florida aboard a United Launch Alliance Atlas V 411 rocket, which includes a 4-meter diameter payload fairing and one solid rocket motor. Only three Atlas V’s have been launched in this configuration.

“In just over 500 days, we will begin our seven-year journey to Bennu and back. This is an exciting time,” said Lauretta.

The spacecraft will reach Bennu in 2018 and return a sample to Earth in 2023.

Bennu is an unchanged remnant from the collapse of the solar nebula and birth of our solar system some 4.5 billion years ago, little altered over time.

The Atlas V with MMS launches, as seen by this camera placed in the front of the launchpad. Copyright © Alex Polimeni — OSIRIS-REx will launch in 2016 on an Atlas V similar to this one lofting NASA’s MMS satellites on March 12, 2015, as seen by this camera placed in the front of the launchpad. Copyright © Alex Polimeni

Significant progress in spacecraft assembly has already been accomplished at Lockheed’s Denver manufacturing facility.

“The spacecraft structure has been integrated with the propellant tank and propulsion system and is ready to begin system integration in the Lockheed Martin highbay,” said Mike Donnelly, OSIRIS-REx project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in a statement.

“The payload suite of cameras and sensors is well into its environmental test phase and will be delivered later this summer/fall.”

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, following New Horizons to Pluto and Juno to Jupiter, which also launched on Atlas V rockets.

The most recent Atlas V launched NASA’s MMS quartet of Earth orbiting science probes on March 12, 2015.

OSIRIS-REx logo

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is responsible for overall mission management.

OSIRIS-REx complements NASA’s Asteroid Initiative – including the Asteroid Redirect Mission (ARM) which is a robotic spacecraft mission aimed at capturing a surface boulder from a different near-Earth asteroid and moving it into a stable lunar orbit for eventual up close sample collection by astronauts launched in NASA’s new Orion spacecraft. Orion will launch atop NASA’s new SLS heavy lift booster concurrently under development.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Artist's concept of the OSIRIS-REx spacecraft collecting a sample from asteroid 1999 RQ36. Credit: NASA — Artist’s concept of the OSIRIS-REx spacecraft collecting a sample from asteroid 1999 RQ36. Credit: NASA

Juno soars skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com — OSIRIS-REx is the 3rd mission in NASA’s New Frontiers program. It follows NASA’s Juno orbiter seen here soaring skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com

April 1, 2015December 23, 2015 by Matt Williams

A Red Moon – NOT a Sign of the Apocalypse!

Composite picture of a dark red Moon during a total lunar eclipse. Credit: NASA/ Johannes Schedler (Panther Observatory)

On most evenings, the Moon will appear as a bright yellow or white color in the night sky. But on occasion, the Moon can turn a beautiful and dramatic red, coppery color. Naturally, there are a number of superstitions associated with this stellar event. But to modern astronomers, a Red Moon is just another fascinating phenomenon that has a scientific explanation.

Since the earliest days of recorded history, the Moon has been believed to have a powerful influence over human and animal behavior. To the Romans, staring at a full Moon was thought to drive a person crazy – hence the term “lunatic”. Farmers in the past would plant their crops “by the moon”, which meant sowing their seeds in accordance with the Moon’s phases in the hopes of getting a better harvest.

So naturally, when the Moon turned red, people became wary. According to various Biblical passages, a Blood Moon was thought to be a bad omen. But of course, the Moon turns red on a semi-regular basis, and the world has yet to drown in fire. So what really accounts for a “Red Moon?” What causes Earth’s only satellite to turn the color of blood?

Ordinarily, the Moon appears as it does because it is reflecting light from the Sun. But on occasion, it will darken and acquire either a golden, copper, or even rusty-red color.

There are few situations that can cause a red Moon. The most common way to see the Moon turn red is when the Moon is low in the sky, just after moonrise or before it’s about to set below the horizon. Just like the Sun, light from the Moon has to pass through a larger amount of atmosphere when it’s down near the horizon, compared to when it’s overhead.

The Earth’s atmosphere can scatter sunlight, and since moonlight is just scattered sunlight, it can scatter that too. Red light can pass through the atmosphere and not get scattered much, while light at the blue end of the spectrum is more easily scattered. When you see a red moon, you’re seeing the red light that wasn’t scattered, but the blue and green light have been scattered away. That’s why the Moon looks red.

The second reason for a red Moon is if there’s some kind of particle in the air. A forest fire or volcanic eruption can fill the air with tiny particles that partially obscure light from the Sun and Moon. Once again, these particles tend to scatter blue and green light away, while permitting red light to pass through more easily. When you see a red moon, high up in the sky, it’s probably because there’s a large amount of dust in the air.

Depiction of the Sun's rays turning the Moon red. Image Credit: NASA/Mars Exploration — *Depiction of the Sun’s rays turning the Moon red. Image Credit: NASA/Mars Exploration*

A third – and dramatic – way to get a red Moon is during a lunar eclipse. This happens when the Moon is full and passes into Earth’s shadow (also known as the umbra), which darkens it. At that point, the Moon is no longer being illuminated by the Sun. However, the red light passing through the Earth’s atmosphere does reach the Moon, and is thus reflected off of it.

For those observing from the ground, the change in color will again be most apparent when the Moon appears low in the night sky, just after moonrise or before it’s about to set below the horizon. Once again, this is because our heavy atmosphere will scatter away the blue/green light and let the red light go straight through.

The reddish light projected on the Moon is much dimmer than the full white sunlight the Moon typically reflects back to us. That’s because the light is indirect and because the red-colored wavelengths are only a part of what makes up the white light from the sun that the Moon usually receives.

In other words, when you see a red Moon, you’re seeing the result of blue and green light that has been scattered away, and the red light remaining.

Path of the Moon through Earth's umbral and penumbral shadows during the Total Lunar Eclipse of April 15, 2014. Image Credit: NASA/Eclipse — *Path of the Moon through Earth’s umbral and penumbral shadows during the Total Lunar Eclipse of April 15, 2014. Image Credit: NASA/Eclipse Website*

And that’s the various ways how we get a Red Moon in the night sky. Needless to say, our ancient forebears were a little nervous about this celestial phenomenon occurrence.

For example, Revelations 6:12/13 says that a Red Moon is a sign of the apocalypse: “When he opened the sixth seal, I looked, and behold, there was a great earthquake, and the sun became black as sackcloth, the full moon became like blood, and the stars of the sky fell to the earth as the fig tree sheds its winter fruit when shaken by a gale.”

But rest assured that if you see one, it’s not the end of the world. The Sun and Moon will rise again. And be sure to check out this Weekly Space Hangout, where the April 4th eclipse is discussed:

We have covered lunar eclipses many times on Universe Today, and often explain the red Moon phenomenon. Here’s another good explanation of the science behind a Red Moon, and why the recent series of lunar eclipses in 2014 and 2015 (known as a tetrad) do not mean anything apocalyptic, and here’s another article about how to see a lunar eclipse. Here’s an article that includes a stunning array of images of the Moon during an eclipse in 2014.

Of course, NASA has some great explanations of the red Moon effect during a lunar eclipse. Here’s another one.

You can listen to a very interesting podcast about the formation of the Moon from Astronomy Cast, Episode 17: Where Did the Moon Come From?

Sources: NASA Science: Lunar Eclipse, NASA: Mars Exploration, Discovery News, NASA: Eclipse Website

April 1, 2015December 23, 2015 by Nancy Atkinson

Gallery: Behind the Scenes Images of the Final Hubble Servicing Mission

Hubble Servicing Mission astronaut training in the water of the Neutral Buoyancy Lab in Houston, Texas, February 2009. Credit and copyright: Michael Soluri.

Photographer Michael Soluri was granted unprecedented access to document the people and events behind the final Hubble Space Telescope Servicing Mission 4, STS-125, which launched in 2009. He has published these images in a new book, “Infinite Worlds: People & Places of Space Exploration.” Soluri has provided Universe Today with an exclusive gallery of images from the book, and also told us about his experiences in being able to follow for three years the behind the scenes lead-up to the mission.

Read his account and see more images below. You can read our full review of Infinite Worlds here.

K. Megan McArthur (PH.D.), the STS-125 Hubble SM4 Robotic Arm engineer during final servicing mission to Hubble, May 2009. Credit and copyright: Michael Soluri.

From a very early age following the space program and over the decades as a documentary photographer on location at various NASA flight centers, I always felt something was missing: an honest, unscripted visual sense of the people behind the scenes that make human and robotic space flight possible.

Yes, it’s always inspiring to experience and photograph a rocket launch with remote equipment or from 3 miles away. However, the access pattern over time has been the same. Writers and photographers herded together into controlled situations that in the end capture the same shot. Given security issues, this is understandable and the results over the decades are predictable.

To achieve the results experienced in Infinite Worlds required earning the trust of both the crew as well as Hubble and shuttle flight management. That trust contributed to being asked by the STS-125 crew to coach them in making better more visually communicative images of their experiences at Hubble. It also enabled me to be a part of and be accepted into the many worlds of that mission during good times and challenging ones.

The edited results comprise my book and exhibitions. Looking back on that journey, I am humbled by the mutual respect and trust extended to me by a remarkable, “made in the USA” labor force that for the most part no longer exists.

— Michael Soluri

Mark Turczyn, Hubble Space Telescope Senior Systems Engineer. In 'Infinite Worlds' he said, ""Every time we ran out of time … we created more." Credit and copyright: Michael Soluri. — Mark Turczyn, Hubble Space Telescope Senior Systems Engineer. In ‘Infinite Worlds’ he said, “”Every time we ran out of time … we created more.” Credit and copyright: Michael Soluri.

Office white-board of Mark Turczyn, HST Senior Systems Engineer. Credit and copyright: Michael Soluri.

Greg Cecil, a Thermal Protection Systems Technician, replaced and caulked damaged tiles on the cockpit area of the space shuttle. He is currently a middle school science teacher. Credit and copyright: Michael Soluri.

Christy Hansen, EVA Task Lead and STS-125 SM4 astronaut Drew Feustel in cargo bay of Atlantis in July 2008. Credit and copyright: Michael Soluri.

Four of the "space-walking" astronauts and their mission trainers reviewing one of the tool boxes they will be accessing in the cargo bay of the shuttle during the last service mission to the Hubble Space Telescope. Credit and copyright: Michael Soluri. — Four of the “space-walking” astronauts and their mission trainers reviewing one of the tool boxes they will be accessing in the cargo bay of the shuttle during the last service mission to the Hubble Space Telescope. Credit and copyright: Michael Soluri.

Mini Power Drill System, designed at NASA Goddard SpaceFlight Center used by astronauts on the final mission to the Hubble Space Telescope, May 2009. Credit and copyright: Michael Soluri.

The astronaut EVA crew of Hubble SM4 - last servicing mission to the Hubble by a space shuttle crew. From left to right: John Grunsfeld, Drew Feustel, Michael Good, and Mike Massimino. Image taken at Goddard Space Flight Center, July 2008. Credit and copyright: Michael Soluri. — The astronaut EVA crew of Hubble SM4 – last servicing mission to the Hubble by a space shuttle crew. From left to right: John Grunsfeld, Drew Feustel, Michael Good, and Mike Massimino. Image taken at Goddard Space Flight Center, July 2008. Credit and copyright: Michael Soluri.

John Grunsfeld, just before entering shuttle Atlantis for his fifth mission in space and his third to the Hubble Space Telescope. Grunsfeld wrote "Climbing Mountains" for Infinite Worlds. Credit and copyright: Michael Soluri. — John Grunsfeld, just before entering shuttle Atlantis for his fifth mission in space and his third to the Hubble Space Telescope. Grunsfeld wrote “Climbing Mountains” for Infinite Worlds. Credit and copyright: Michael Soluri.

Atlantis just after roll out and pad lock down at Pad 39A at Kennedy Space Center for the STS-125 Hubble Servicing Mission. March 31, 2009. Credit and copyright: Michael Soluri.

Jill McGuire, Manager, Hubble SM4 Crew Aids and Tools, in Mission control in Houson during EVA 4, May 2009. Credit and copyright: Michael Soluri.

Self Portrait by John Grunsfeld and shuttle Atlantis on the Hubble Space Telescope -- orbiting Earth. Image courtesy Michael Soluri. — Self Portrait by John Grunsfeld and shuttle Atlantis on the Hubble Space Telescope — orbiting Earth. Image courtesy Michael Soluri.

Several of Soluri’s images of the SM4’s EVA tools and photos by the Atlantis crew are part of an exhibition at the Smithsonian Air and Space Museum Outside the Spacecraft: 50 Years of Extra-Vehicular Activity, on view at the Air and Space Museum through June 8. There’s also an online exhibition. Smithsonian Associates is the presenting organization.

Soluri will give a presentation and do a book signing on April 11, 2015 at the Smithsonian’s Hirshhorn Museum & Sculpture Garden. Soluri will be joined by four individuals who played key roles in Service Mission SM4: astronaut Scott Altman, the STS-125 shuttle commander; David Leckrone, senior project scientist; Christy Hansen, EVA spacewalk flight controller and astronaut instructor; and Hubble systems engineer Ed Rezac. More information on that event can be found here.

April 1, 2015December 23, 2015 by Tyler Simko

Book Review: “Infinite Worlds: People & Places of Space Exploration” by Michael Soluri

Infinite Worlds - People & Places of Space Exploration: by Michael Soluri, Foreword by John Glenn. Cover image courtesy of Michael Soluri and Simon & Schuster.

On April 24, 1990, the Hubble Space Telescope was launched from Kennedy Space Center into low Earth orbit. Hubble was the first telescope designed to operate in space, so it was able to avoid interference from Earth’s atmosphere – an inconvenience that had limited astronomers since they first looked up to the skies. However, scientists quickly realized that something was wrong; the images were blurry. Despite being among the most precisely ground instruments ever made, the primary mirror in the Hubble was about 2,200 nanometers too flat at the perimeter (for reference, the width of a typical sheet of paper is about 100,000 nanometers). Luckily, there was a solution.

Hubble was designed to be serviced in space. As NASA writes on the telescope’s website, “a series of small mirrors could be used to intercept the light reflecting off the mirror, correct for the flaw, and bounce the light to the telescope’s science instruments.” A series of five missions lasting from 1993 to 2009 was devised to correct the mirror and perform various upgrades. Despite being the first of their kind, the missions were declared a resounding success – and they enabled the Hubble Space Telescope to remain operational to this day. Many of Hubble’s images are among the most incredible ever produced by mankind, yet few people know anything about the remarkable men and women who made them possible.

ohn Grunsfeld, just before entering shuttle Atlantis for his fifth mission in space and his third to the Hubble Space Telescope. Grunsfeld wrote "Climbing Mountains" for Infinite Worlds. Credit and copyright: Michael Soluri. — ohn Grunsfeld, just before entering shuttle Atlantis for his fifth mission in space and his third to the Hubble Space Telescope. Grunsfeld wrote “Climbing Mountains” for Infinite Worlds. Credit and copyright: Michael Soluri.

See an exclusive gallery of images from the book here.

Infinite Worlds: People & Places of Space Exploration, the latest book from photographer Michael Soluri, documents the people who worked on the last of these repair missions, STS-125 (also known as Hubble Space Telescope Servicing Mission 4 [HST-SM4]). The nearly two-week journey aboard Space Shuttle Atlantis saw the successful installation of two new instruments and the repair of two others. Like the four other shuttle crews that came before them, the men and women aboard STS-125 enabled Hubble to see deeper and farther into the past than ever before.

Michael Massimino, a veteran of the earlier STS-109 mission, is one of these people. Massimino and Soluri became fast friends after a chance encounter, when Soluri asked: “What is the quality of light really like in space?” Following their discussion, Massimino asked Soluri to teach him and the rest of the crew how to take photographs that would better communicate their experiences in space. Astronauts are always taking pictures, but the lighting in space is, understandably, not always ideal. Like Soluri himself in Infinite Worlds, the astronauts repairing Hubble were looking for better ways to communicate the beauty of space travel through photography.

Soluri was granted unprecedented access to document the people and events behind the mission throughout a period of more than four years. The photographs in the book “give deserved attention to a few of the many thousands of people who worked on the Space Shuttle and Hubble Space Telescope programs,” reads an inspiring foreword by John Glenn, the first American to orbit the Earth. Infinite Worlds reveals a side of space travel that most of us would never otherwise see, including the training sessions, tools, and trials that make success possible. NASA, notorious for keeping their employees tightly scripted and inaccessible, rarely grants such access – and with the closing of the Space Shuttle Program in 2011, such intimacy may never be seen again.

Science is a cooperative discipline, but most people only ever see the results. The tireless work of thousands of individuals is often taken for granted and forgotten. Although many people still hold the false idea that scientific accomplishments are made by individual geniuses working in an armchair, now more than ever before we are entering an age where science is performed by large teams working cooperatively. To mention just one example, CERN hosts scientists of more than 100 nationalities. As Jill McGuire, a manager at Goddard Space Flight Center, writes about the field in the book, “the best way to move forward in the business was to get my hands dirty by working with the skilled machinists and technicians in the branch to learn everything I could.”

Infinite Worlds grants readers an exhilarating glimpse into this cooperative world. One particularly inspiring section follows the immediate buildup to the launch of STS-125. The transcript of the pre-launch quality check is paralleled by images of the situation as it happened. Black and white photographs from both cockpit and control room highlight the tension behind “the most risky thing NASA does,” according to Space Shuttle Launch Director Michael Leinbach. He continues, “they were real people with real families, real children, real lives.” Infinite Worlds reminds us of this: the work behind every scientific breakthrough is not magic, but rather the result of talented and dedicated individuals.

As we approach the 25th anniversary of the Hubble Space Telescope’s launch and look to the future, a book like Infinite Worlds is more relevant now than ever before. The beautiful photographs in Soluri’s book tell two kindred stories: not only the heroic report of repairing a multi-billion dollar piece of equipment, but also a unique glimpse at the inspiring men and women who made it all possible. Whether humanity’s next missions are to Mars, Europa, or elsewhere, one thing will remain constant – we will only reach the stars through the work of exceptional people.

Infinite Worlds is available at Amazon, Barnes and Noble, Indiebound, iBooks, and Google Play.

Learn more about Michael Soluri at his website.

Several of Soluri’s images of the SM4’s EVA tools and photos by the Atlantis crew are part of an exhibition at the Smithsonian Air and Space Museum, Outside the Spacecraft: 50 Years of Extra-Vehicular Activity, on view at the Air and Space Museum through June 8. There’s also an online exhibition.

April 1, 2015December 23, 2015 by Nancy Atkinson

Eye of Super Typhoon Maysak Looks “Like a Black Hole” from Space

Maysak, a category 4 Super Typhoon, as photographed by astronaut Terry Virts on board the International Space Station. Credit: NASA/Terry Virts.

From his perch on the International Space Station, astronaut Terry Virts has been taking some beautiful photos of Earth and space and sharing them on social media. Today, he shared his views of Super Typhoon Maysak, including this terrifying view looking straight down into the huge eye of the storm. “Looking down into the eye – by far the widest one I’ve seen,” he tweeted. “It seemed like a black hole from a Sci-Fi movie.”

See more of his images, below.

According to AccuWeather.com, Super Typhoon Maysak is one of the strongest cyclones in history during the months of January, February and March. It has slammed several Micronesian islands, killing 5 people, and is now on its way to the Philippines. As of early on April 1, Maysak had sustained winds of 240 kph (150 mph), equivalent of a Category 4 hurricane. Gusts as high as 390 kph (180 mph) are possible with this storm.

Looking down into the eye – by far the widest one I’ve seen. It seemed like a black hole from a Sci-Fi movie #Maysak pic.twitter.com/hmdBStaY6r

— Terry W. Virts (@AstroTerry) April 1, 2015

The eye of #Maysak typhoon really stands out early in the morning with the shadow being cast deep into the vortex pic.twitter.com/SodkijMt7O

— Terry W. Virts (@AstroTerry) April 1, 2015

More views of the eye- this was about 12 hours ago at sunrise, local time. Unbelievable. #Maysak pic.twitter.com/9Z6obnSVjh

— Terry W. Virts (@AstroTerry) April 1, 2015

The typhoon is expected to weaken, but still poses a threat to the islands in its path:

A graphic showing Typhoon Maysak's projected path. Credit: AccuWeather.com — A graphic showing Typhoon Maysak’s projected path. Credit: AccuWeather.com

March 31, 2015December 23, 2015 by Nancy Atkinson

Stunning Photo of Volcanic Lightning at Volcán de Colima in Mexico

The Colima Volcano (Volcán de Colima) pictured on March 29, 2015 with lightning. Credit and copyright: César Cantú.

The Colima volcano in Mexico is active again, and has been spewing out large plumes of ash nearly 3 kilometers into the air. Astrophotographer César Cantú captured this spectacular picture of lightning slicing through the cloud of ash.

How can lightning strike in an ash cloud? Through friction, particles of the ash can charge each other by rubbing against each other during the eruption. When the energy is discharged, it can create lightning bolts.

The Colima volcano is one of the most active volcanoes in Mexico, and is also called ‘Volcán de Fuego’ or ‘Fire volcano.’ It has erupted more than 40 times since the first documented eruption in 1576.

The latest news on this current eruption is that local authorities have put the volcano on a yellow alert, meaning the volcano is showing increased activity, and residents who live nearby should prepare for a possible evacuation.

Stay safe César, and thanks for sharing your image with Universe Today! See a larger version on his website here.

March 31, 2015December 23, 2015 by David Dickinson

Seeking Ceres: Following the Brave New World Through 2015

A little world is making big headlines in 2015. NASA’s Dawn spacecraft entered orbit around 1 Ceres on March 6^th, 2015, gaving us the first stunning images of the ~900 kilometre diameter world. But whether you refer to Ceres as a dwarf planet, minor planet, or the king of the asteroid belt, this corner of the solar system’s terra incognita is finally open for exploration. It has been a long time coming, as Ceres has appeared as little more than a wandering, star-like dot in the telescopes of astronomers for over two centuries since discovery.

Untitled — The orbit of 1 Ceres. Credit: NASA/JPL

And the good news is, you can observe Ceres from your backyard if you know exactly where to look for it with binoculars or a small telescope. We’ll admit, we had an ulterior motive on pulling the trigger on this post three months prior to opposition on July 24th, as Dawn will soon be exiting its ‘shadow phase’ and start unveiling the world to us up close. The first science observations for Dawn begin in mid-April.

Ceres spends all of 2015 looping through the constellations of Capricornus, Microscopium and Sagittarius. This places it low to the south for northern hemisphere observers on April 1^st in the early morning sky. Ceres will pass into the evening sky by mid-summer. Ceres orbits the Sun once every 4.6 years in a 10.6 degree inclination path relative to the ecliptic that takes it 2.6 AU to 3 AU from the Sun. The synodic period of Ceres is, on average, 467 days from one opposition to the next.

Shining at magnitude +8, April 1^st finds Ceres near the Capricornus/Sagittarius border. Ceres can reach magnitude +6.7 during a favorable opposition. Note that Ceres is currently only 20 degrees east of the position of Nova Sagittarii 2015 No. 2, currently still shining at 4th magnitude. June 29th and November 25th are also great times to hunt for Ceres in 2015 as it loops less than one degree past the 4^th magnitude star Omega Capricorni.

June 30 — Ceres meets up with Omega Capricorni on June 29th. Credit: Stellarium.

You can nab Ceres by carefully noting its position against the starry background from night to night, either by sketching the suspect field, or photographing the region. Fans of dwarf planets will recall that 1 Ceres and 4 Vesta fit in the same telescopic field of view last summer, and now sit 30 degrees apart. Ceres is now far below the ecliptic plane, but will resume getting occulted by the passing Moon on February 3^rd, 2017.

Left — The Palermo transit instrument used to discover Ceres. From *Della Specola Astronomica* (1792)

Ceres was discovered by Giuseppe Piazzi on the first day of the 19^th century on January 1^st, 1801. Ceres was located on the Aries/Cetus border just seven degrees from Mars during discovery. Piazzi wasn’t even on the hunt for new worlds at the time, but was instead making careful positional measurements of stars with the 7.5 centimetre Palermo Circle transit telescope.

At the time, the discovery of Ceres was thought to provide predictive proof of the Titus-Bode law: here was a new planet, just where this arcane numerical spacing of the planets said it should be. Ceres, however, was soon joined by the likes of Juno, Pallas, Vesta and many more new worldlets, as astronomers soon came to realize that the solar system was not the neat and tidy place that it was imagined to be in the pre-telescopic era.

To date, the Titus-Bode law remains a mathematical curiosity, which fails to hold up to the discovery of brave new exoplanetary systems that we see beyond our own.

The view from Ceres itself would be a fascinating one, as an observer on the Cererian surface would be treated to recurrent solar transits of interior solar system worlds. Mercury would be the most frequent, followed by Venus, which transits the Sun as seen from Ceres 3 times in the 21^st century: August 1^st, 2042, November 19^th, 2058 and February 13^th 2068. Mars actually transits the Sun as seen from Ceres even earlier on June 9^th, 2033. Curiously, we found no transits of the Earth as seen from Ceres during the current millennium from 2000 to 3000 AD!

From Ceres, Jupiter would also appear 1.5’ in diameter near opposition, as opposed to paltry maximum of 50” in size as seen from the Earth. This would be just large enough for Jupiter to exhibit a tiny disk as seen from Ceres with the unaided eye. The four major Galilean moons would be visible as well.

The mysteries of Ceres beckon. Does the world harbor cryovolcanism? Just what are those two high albedo white dots? Are there any undiscovered moons orbiting the tiny world? If a fair amount of surface ice is uncovered, Ceres may soon become a more attractive target for human exploration than Mars.

All great thoughts to ponder, as this stellar speck in the eyepiece of your backyard telescope becomes a brand new world full of exciting possibilities.

March 31, 2015December 28, 2015 by Susie Murph

Carnival of Space #398-399

Carnival of Space. Image by Jason Major.

This week’s Carnival of Space is hosted by Brian Wang at his Next Big Future blog.

Click here to read Carnival of Space #399

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.