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NinjaSat: A Small Satellite's Big Impact

NinjaSat is changing space science with innovative X-ray observations.

Toru Tamagawa, Teruaki Enoto, Takao Kitaguchi, Wataru Iwakiri, Yo Kato, Masaki Numazawa, Tatehiro Mihara, Tomoshi Takeda, Naoyuki Ota, Sota Watanabe, Amira Aoyama, Satoko Iwata, Takuya Takahashi, Kaede Yamasaki, Chin-Ping Hu, Hiromitsu Takahashi, Yuto Yoshida, Hiroki Sato, Shoki Hayashi, Yuanhui Zhou, Keisuke Uchiyama, Arata Jujo, Hirokazu Odaka, Tsubasa Tamba, Kentaro Taniguchi

― 6 min read


NinjaSat: Mighty X-Ray NinjaSat: Mighty X-Ray Explorer astronomy. A small satellite revolutionizes X-ray
Table of Contents

NinjaSat is a small satellite designed to study X-ray sources in space. Launched on November 11, 2023, this 6U CubeSat aims to observe some of the brightest X-ray sources in the universe, like a tiny spy peeking into the secrets of the cosmos. Weighing only 8 kg, NinjaSat packs a punch when it comes to observing celestial objects, helping scientists gather valuable Data over time.

The Need for NinjaSat

For decades, space science has been led by large agencies that send big Satellites into space. This approach has produced many discoveries but comes with high costs and long waiting times. It's a bit like trying to book a fancy restaurant where the waitlist is longer than the meal itself! Meanwhile, the demand for more sensitive telescopes is on the rise, and scientists are eager to find quicker ways to conduct research.

In the last ten years, private companies have entered the arena, building smaller and more affordable satellites. NinjaSat aims to take advantage of this trend and show that small satellites can achieve significant scientific outcomes. Think of it as a nimble sports car zipping through traffic while the bigger vehicles struggle to change lanes.

Design and Features

NinjaSat is like the Swiss Army knife of satellites. Its design allows it to perform various Observations from a size that fits in the palm of your hand. The satellite can accurately point at X-ray sources using a method called three-axis attitude control. This ensures that its observations are precise and reliable.

The Satellite Bus

The backbone of the NinjaSat is a commercial satellite bus made by NanoAvionics. This bus serves as the satellite's body and houses all the necessary components for operations. It’s like choosing a sturdy backpack for a camping trip—you need it to carry all your gear without falling apart.

NinjaSat's bus is equipped with two non-imaging gas X-ray detectors that can observe X-ray energy in the range of 2–50 keV. With its effective area of 32 cm² at 6 keV, NinjaSat can observe X-ray sources that are quite faint. The satellite also tags each photon with a time resolution of 61 microseconds, allowing scientists to track them accurately.

Monitoring Protectors

NinjaSat comes with built-in radiation belt Monitors that measure the flux of protons and electrons in its orbit. These monitors alert the X-ray detectors if the radiation exceeds certain levels, ensuring that the satellite can protect itself from potentially damaging particles. It’s like an early warning system that keeps the satellite safe, much like a fire alarm in a kitchen.

The Mission Objectives

NinjaSat's mission objectives are straightforward but ambitious. This satellite aims to conduct X-ray observations using compact scientific instruments, detecting X-rays from specific celestial objects.

Minimum Success

The minimum success criteria involve pointing at an X-ray source and successfully detecting X-rays from it. This is the baseline goal set to demonstrate the satellite's capabilities.

Full Success

Full success will be achieved if NinjaSat observes at least two X-ray sources and publishes two scientific papers. It’s like passing a final exam and being able to brag about it!

Extra Success

Extra success involves one of two additional outcomes: conducting simultaneous observations with other telescopes to make exciting discoveries or measuring the rotation period of a nearby neutron star to help find gravitational waves. Think of this as leveling up in a video game—achievements get more impressive as you go!

Timeline of Development

The NinjaSat project kicked off in 2020, and like any good story, it faced some challenges along the way. Fabrication of the scientific payloads wrapped up in August 2022, with satellite assembly and testing completed in July 2023. Finally, it was launched into space in the bustling month of November 2023.

Launch Day

On launch day, the excitement was palpable! NinjaSat was part of a ride-along mission with numerous other satellites. You could imagine all the tiny astronauts waving goodbye as they were launched into the great beyond. The satellite entered a Sun-synchronous orbit, which keeps it in a position where it receives consistent sunlight.

Initial Operations

Once NinjaSat was in orbit, it went through a commissioning phase. This included verifying all systems were operational. It was like a new homeowner checking if all the lights work and the plumbing is good.

First Observations

After about three months of initial operations, NinjaSat turned its gaze toward the Crab Nebula on February 9, 2024. The satellite detected a pulse from the neutron star, marking the achievement of its minimum success criteria. It’s kind of like getting an “A” on your first test!

Scientific Goals

NinjaSat’s main goal is to observe X-ray sources, gathering information about their behavior and characteristics. The project will help contribute to a growing field called time-domain astronomy.

Bright X-ray Sources

Many bright X-ray sources are scattered throughout the universe. For NinjaSat, these sources can be observed continuously, allowing scientists to study their variations over time. Think of it like watching a soap opera unfold in real-time instead of hearing about it from friends!

Communication with Earth

NinjaSat communicates with ground stations using UHF and S-band frequencies. The main ground station is located in Svalbard, Norway, with another one in New Zealand as a backup. This setup ensures that NinjaSat can maintain a connection with its operators back on Earth.

Data and Telemetry

Data collected from observations is sent back to Earth for analysis. These data packets contain valuable information that scientists can use to learn more about the X-ray sources NinjaSat is observing. The satellite downlinks data three times a day, allowing for regular updates.

Managing Risks

Operating a satellite is risky business. To reduce the chances of failure, NinjaSat's team outsourced the satellite bus development to NanoAvionics, which specializes in making small satellites. This partnership allows the scientific team to concentrate on the payload and observations without single-handedly managing the entire satellite's operation.

Conclusion

NinjaSat represents a shift in how we think about space science. It shows that smaller satellites can still make significant contributions to our understanding of the universe. NinjaSat is like a clever little ninja, sneaking around space to deliver valuable data without the need for a massive budget or grandiose plans.

With successful observations already gathered, NinjaSat is poised to continue exploring X-ray sources and contributing to the scientific community. So, the next time someone mentions a small satellite, remember that NinjaSat is not just small—it's mighty in its quest to uncover the mysteries of X-ray astronomy!

Original Source

Title: NinjaSat: Astronomical X-ray CubeSat Observatory

Abstract: NinjaSat is an X-ray CubeSat designed for agile, long-term continuous observations of bright X-ray sources, with the size of 6U ($100\times200\times300$ mm$^3$) and a mass of 8 kg. NinjaSat is capable of pointing at X-ray sources with an accuracy of less than $0^{\circ}\hspace{-1.0mm}.1$ (2$\sigma$ confidence level) with 3-axis attitude control. The satellite bus is a commercially available NanoAvionics M6P, equipped with two non-imaging gas X-ray detectors covering an energy range of 2-50 keV. A total effective area of 32 cm$^2$ at 6 keV is capable of observing X-ray sources with a flux of approximately 10$^{-10}$ erg cm$^{-2}$ s$^{-1}$. The arrival time of each photon can be tagged with a time resolution of 61 $\mu$s. The two radiation belt monitors continuously measure the fluxes of protons above 5 MeV and electrons above 200 keV trapped in the geomagnetic field, alerting the X-ray detectors when the flux exceeds a threshold. The NinjaSat project started in 2020. Fabrication of the scientific payloads was completed in August 2022, and satellite integration and tests were completed in July 2023. NinjaSat was launched into a Sun-synchronous polar orbit at an altitude of about 530 km on 2023 November 11 by the SpaceX Transporter-9 mission. After about three months of satellite commissioning and payload verification, we observed the Crab Nebula on February 9, 2024, and successfully detected the 33.8262 ms pulsation from the neutron star. With this observation, NinjaSat met the minimum success criterion and stepped forward to scientific observations as initially planned. By the end of November 2024, we successfully observed 21 X-ray sources using NinjaSat. This achievement demonstrates that, with careful target selection, we can conduct scientific observations effectively using CubeSats, contributing to time-domain astronomy.

Authors: Toru Tamagawa, Teruaki Enoto, Takao Kitaguchi, Wataru Iwakiri, Yo Kato, Masaki Numazawa, Tatehiro Mihara, Tomoshi Takeda, Naoyuki Ota, Sota Watanabe, Amira Aoyama, Satoko Iwata, Takuya Takahashi, Kaede Yamasaki, Chin-Ping Hu, Hiromitsu Takahashi, Yuto Yoshida, Hiroki Sato, Shoki Hayashi, Yuanhui Zhou, Keisuke Uchiyama, Arata Jujo, Hirokazu Odaka, Tsubasa Tamba, Kentaro Taniguchi

Last Update: 2024-12-03 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2412.03016

Source PDF: https://arxiv.org/pdf/2412.03016

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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