OrbitalHub

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The Neutron Star Interior Composition Explorer (NICER) is a NASA mission launched in June 2017 and mounted on the International Space Station (ISS). Its primary objective is to study neutron stars—ultra-dense remnants of massive stars that have undergone supernova explosions. By observing X-ray emissions from these celestial objects, NICER aims to provide insights into their internal structures and the fundamental physics governing matter under extreme conditions.

NICER’s core component is the X-ray Timing Instrument (XTI), designed for high-precision timing and spectroscopy of soft X-rays in the 0.2–12 keV energy range. The XTI comprises 56 co-aligned X-ray concentrator optics, each paired with a silicon drift detector. These concentrators utilize grazing-incidence optics with 24 nested mirrors to focus incoming X-rays onto their respective detectors, enhancing sensitivity and resolution.

NICER is mounted on the ISS’s ExPRESS Logistics Carrier-2. It features a two-axis pointing system that allows the instrument to track celestial targets across the sky. An integrated star tracker ensures precise alignment, enabling NICER to observe multiple targets during each 92-minute orbit of the ISS.

To achieve its scientific goals, NICER incorporates a GPS-based timing system capable of tagging photon arrival times with sub-microsecond accuracy. This high temporal resolution is crucial for studying the rapid rotational periods of pulsars and other time-sensitive phenomena.

NICER has significantly advanced our understanding of neutron star interiors by providing precise measurements of their masses and radii. These observations have helped constrain the equation of state for ultra-dense matter, shedding light on the behavior of matter at densities exceeding those found in atomic nuclei.

An extension of NICER’s mission, known as SEXTANT (Station Explorer for X-ray Timing and Navigation Technology), successfully demonstrated the use of X-ray pulsars for autonomous spacecraft navigation. By measuring the timing of X-ray pulses from known pulsars, SEXTANT was able to determine the ISS’s position in space, paving the way for future deep-space navigation systems.

In 2018, NICER discovered an X-ray pulsar in the fastest known stellar orbit, with a companion star completing an orbit every 38 minutes. This finding provides valuable data on the dynamics of compact binary systems and the extreme gravitational environments in which they exist.

NICER observed the brightest X-ray burst ever recorded from the neutron star SAX J1808.4−3658. This event offered insights into thermonuclear processes on neutron star surfaces and the mechanisms driving such energetic emissions.

Although primarily focused on neutron stars, NICER has also contributed to black hole research. It mapped “light echoes” from the stellar-mass black hole MAXI J1820+070, revealing changes in the size and shape of the surrounding accretion disk and corona. These observations enhance our understanding of black hole accretion processes and their immediate environments.

In May 2023, NICER’s thermal shields developed a leak, allowing stray light to interfere with its X-ray detectors. To address this issue, NASA designed specialized patches delivered to the ISS via the Cygnus NG-21 resupply mission in August 2024. Astronauts successfully applied these patches during a spacewalk on January 16, 2025, restoring NICER’s full observational capabilities.

As of early 2025, NICER has contributed to over 300 scientific publications, underscoring its significant role in advancing astrophysical research. Its high-precision measurements continue to provide valuable data for the scientific community, enhancing our understanding of neutron stars and other cosmic phenomena.

Video credit: NASA Goddard

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SpaceX’s Fram2 mission, launched on March 31, 2025, from Kennedy Space Center, marked a historic milestone as the first human spaceflight to orbit over Earth’s polar regions. This privately funded mission, led by cryptocurrency entrepreneur Chun Wang, featured a diverse international crew and aimed to advance scientific research and exploration.

The mission’s name, Fram2, pays homage to the Norwegian exploration ship Fram, symbolizing a new era of polar exploration—this time from space. The spacecraft completed multiple orbits over both the North and South Poles, providing unprecedented views and data.

The crew members are:

Chun Wang (Mission Commander): A Maltese entrepreneur of Chinese origin and founder of F2Pool, Wang financed the mission.

Jannicke Mikkelsen (Capsule Commander): A Norwegian cinematographer specializing in extreme environments.

Rabea Rogge (Pilot): A German robotics researcher and the first German woman in space.

Eric Philips (Mission Specialist & Medical Officer): An Australian polar explorer and guide.

All crew members were civilians with backgrounds in exploration and science, emphasizing the mission’s pioneering spirit.

The Fram2 mission conducted 22 experiments focusing on:

Human Physiology: Including the first X-ray of a human in space and studies on blood flow restriction to mitigate muscle and bone loss in microgravity.

Radiation Exposure: Assessing the effects of increased cosmic radiation encountered in polar orbits.

Biological Studies: Attempting to cultivate oyster mushrooms in space as a potential food source.

Atmospheric Phenomena: Observing aurora-like events such as STEVE and green emissions using high-resolution cameras.

Educational Outreach: The “Fram2Ham” amateur radio project connected with students worldwide, promoting STEM education.

Mission Highlights

Historic Polar Orbit: Fram2 was the first crewed mission to achieve a polar orbit, offering unique perspectives of Earth’s poles.

International Collaboration: The diverse crew underscored the global nature of modern space exploration.

Scientific Contributions: The mission’s experiments provided valuable data for future long-duration spaceflights.

Cultural Significance: Artifacts such as a piece of the original Fram ship’s deck and a Stephen Hawking Medal were carried onboard, bridging past and future explorations.

Fram2’s success demonstrates the potential of private missions to contribute meaningfully to space science and exploration. By achieving a polar orbit, the mission opened new avenues for Earth observation and research. The data collected will inform future missions, particularly those targeting long-duration travel to destinations like Mars. Moreover, the mission’s emphasis on international cooperation and educational outreach sets a precedent for inclusive and globally beneficial space endeavors.

Video credit: SpaceX

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Engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, recently completed a test fire campaign of a 14-inch hybrid rocket motor. The rocket motor ignites using both solid fuel and a stream of gaseous oxygen to create a powerful stream of rocket exhaust. Data from the test campaign will help teams prepare for future flight conditions when commercial human landing systems, provided by SpaceX and Blue Origin, touch down on the Moon for crewed Artemis missions.

The hybrid motor was test fired 30 times to ensure it will reliably ignite in preparation for testing later this year at NASA’s Langley Research Center in Hampton, Virginia. This video shows the 28th test, conducted in February, during which the 3D-printed motor fired for six seconds.

Video credit: NASA’s Marshall Space Flight Center

NASA dicit:

​Technicians use massive cranes inside the Vehicle Assembly Building at NASA Kennedy’s Space Center in Florida to lift the fully assembled SLS (Space Launch System) core stage vertically 225-feet above the ground from High Bay 2 to a horizontal position in the facility’s transfer aisle. In the transfer aisle, technicians conducted final preparations of the core stage before it was integrated with the completed twin solid rocket booster segments. NASA is implementing a more efficient stacking process to support future missions to the Moon beginning with the Artemis II test flight.

Video credit: NASA

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NASA’s Lucy mission, launched on October 16, 2021, is the first space mission specifically designed to study the Trojan asteroids, a unique group of asteroids that orbit the Sun in two large swarms around Jupiter—one leading and one trailing the gas giant. These celestial bodies are believed to be remnants from the early solar system, offering valuable clues about the formation of the planets. Named after the fossilized human ancestor “Lucy,” whose discovery shed light on human evolution, this spacecraft similarly seeks to uncover the ancient history of the solar system.

The Lucy mission has four primary scientific goals:

Surface Geology – Analyze surface features to determine the history of cratering, layering, and possible past activity like volcanism.

Surface Composition – Identify the composition of the asteroids’ surfaces to infer the origins of their materials.

Interior and Bulk Properties – Measure mass, density, and structure of each asteroid to understand their internal makeup.

Satellites and Rings – Search for small moons and ring systems, which may help scientists understand how Trojan asteroids have evolved.

By studying these diverse objects, Lucy is expected to provide insights into planetary formation processes and the dynamics of the early solar system.

Lucy’s mission trajectory is one of the most complex ever attempted. It involves multiple gravity assists and a looping journey through the inner solar system to reach different groups of Trojan asteroids. After launching from Cape Canaveral aboard an Atlas V rocket, Lucy began a 12-year journey involving three Earth gravity assists:

First Earth flyby: October 2022

Second Earth flyby: December 2024

Third Earth flyby: December 2030

These assists help shape Lucy’s path to visit eight asteroids in total—a record for a single NASA mission. These include:

Donaldjohanson (Main Belt asteroid, 2025) – Named after the discoverer of the Lucy hominid fossil.

Eurybates and its satellite Queta (leading Trojan swarm, 2027)

Polymele (2027)

Leucus (2028)

Orus (2028)

Patroclus and Menoetius (binary pair in the trailing Trojan swarm, 2033)

The spacecraft’s ability to fly by both leading and trailing Trojan camps is made possible by its unique and precisely calculated orbit, using Earth’s gravity to slingshot itself across vast distances.

To fulfill its objectives, Lucy is equipped with a suite of three main science instruments:

L’LORRI (Lucy LOng Range Reconnaissance Imager): A high-resolution telescopic camera designed to capture detailed images of the surface features of the Trojan asteroids, similar to what New Horizons used for Pluto.

L’Ralph: This instrument includes both a color visible camera and an infrared spectrometer to analyze surface composition and detect ices, organics, and minerals.

L’TES (Lucy Thermal Emission Spectrometer): Measures the heat emitted from asteroid surfaces, helping scientists estimate the texture and composition of the materials.

In addition to these, Lucy uses a high-gain antenna and radio tracking to precisely measure the gravitational tug of the asteroids during flybys—key for calculating mass and internal structure.

The mission timeline is as follows:

Launch: October 16, 2021

Earth Flyby 1: October 2022 (completed successfully)

Main Belt asteroid Donaldjohanson flyby: April 2025

Trojan flybys (Eurybates, Queta, Polymele, Leucus, Orus): 2027–2028

Return to Earth for gravity assist: December 2030

Patroclus and Menoetius (binary system) flyby: March 2033

End of Primary Mission: Late 2033 (though the spacecraft may continue as an extended mission platform depending on health and power)

NASA’s Lucy mission is a bold and pioneering effort to study some of the oldest and most distant relics of our solar system. Through its ambitious trajectory and carefully selected instruments, Lucy will give scientists an unprecedented look into the origins and evolution of our planetary neighborhood. By exploring a diverse array of Trojan asteroids—each with its own unique story—Lucy stands to revolutionize our understanding of how the planets formed and why our solar system looks the way it does today.

Video credit: NASA Goddard

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​NASA astronaut Don Pettit, along with Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner, successfully concluded a 220-day mission aboard the International Space Station (ISS) with a safe landing in Kazakhstan on April 20, 2025. Their spacecraft, Soyuz MS-26, touched down southeast of Dzhezkazgan at 6:20 a.m. local time (9:20 p.m. EDT on April 19), coinciding with Pettit’s 70th birthday.​

The trio launched from the Baikonur Cosmodrome on September 11, 2024, and participated in Expeditions 71 and 72. During their time on the ISS, they orbited Earth 3,520 times, covering approximately 93.3 million miles.​

Throughout the mission, the crew conducted various scientific experiments. Pettit focused on enhancing in-orbit metal 3D printing capabilities, advancing water sanitization technologies, exploring plant growth under varying water conditions, and investigating fire behavior in microgravity.​

Following their return, the crew underwent routine medical evaluations. Pettit was transported to NASA’s Johnson Space Center in Houston, while Ovchinin and Vagner returned to the Gagarin Cosmonaut Training Center in Star City, Russia.​

Video credit: NASA