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13 Stech FerSat - unizg.hrscience.geof.unizg.hr/copernicus/Downloads/13_FERSAT project.pdf7huwldu\...

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FERSAT project prof. dr. sc. Dubravko Babić, Objective: Launch 1U CubeSat with a selection of scientific payloads and engineering demonstrations Funding and resources: Croatian Science Foundation (HRZZ IP-2018) Collaboration with other departments at FER, other Faculties at the University of Zagreb, and Croatian industry (Croatel d.o.o, Geolux d.o.o) Multiple donations from Croatian industry A dozen faculty and 70 students are involved
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Page 1: 13 Stech FerSat - unizg.hrscience.geof.unizg.hr/copernicus/Downloads/13_FERSAT project.pdf7huwldu\ sd\ordgv 6sdfh uhdglqhvv ri 3xuh%ghwhfwruv 3xuh%ghwhfwruv duh ghwhfwruv iru hohfwurqv

FERSAT projectprof. dr. sc. Dubravko Babić,

Objective: Launch 1U CubeSat with a selection of scientific payloads and engineering demonstrations

Funding and resources: Croatian Science Foundation (HRZZ IP-2018) Collaboration with other departments at FER,

other Faculties at the University of Zagreb, and Croatian industry (Croatel d.o.o, Geolux d.o.o)

Multiple donations from Croatian industry A dozen faculty and 70 students are involved

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FERSAT nanosatellite

Cube-shaped satelite withvolume of 1 liter and mass ≤ 1.33 kg.

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Planned FERSAT orbit

• Sun-synchronous orbit at altitude 500 – 650 km

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Satellite project components:

Building an Earth station

Building a satellite Satellite Launch

Operation phaseData download, analysis, adapting satelite functions

JiV3

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Slajd 4

JiV3 Bulding/establishing Earth stationJosip i Vedrana, 10-Dec-18

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Primary payload: Light pollution measurement• The type of illumination is changing in the world: from conventional

sodium/Mercury lighting, people are moving to solid-state ligthing (LED).

• Question: Can we get an estimate of what fraction of global lighting has been converted to LEDs?

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The problem

Solid-state lighting exhibits an unnaturally high intensity of blue light. Blue light in the night disturbs animal behavior and human circadian rhythm.

Our objectives:

• Develop an algorithm to provide the fractional contribution of solid-state lighting in the overall world illumination from spectrally resolved images from FERSAT and existing satellites.

• Demonstrate that this can be done efficiently and inexpensively using a CCD camera on a 1U CubeSat.

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Secondary payload: Implement X-band downlink

• CubeSat downlinks are generally in the VHF/UHF amateur radio band and it typically takes 6 satellite passes to download 2MPixel image.

• Question: Can we speed this up to download tens or hundreds of images per satellite pass?

The objective:

• Demonstrate high data-rate X-band communication between 1UCubeSat and Earth station.

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Secondary payload: the approachThe challenge:

• CubeSat thermal budget is very limited, while X-band transmitters dissipate a lot of power (several Watts).

The approach

• Design and implement highly efficient X-band transmitter

• Optimize the link budget.

• Optimize satellite energy management for short-term emission.

Link budget at 8 GHz

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X-band Earth receiverThe challenge:

• Build a high-precision X/Y antenna with an X-band receiver

The approach

• Use 2.4-m elliptical dish with X-band receiving electronics

– In collaboration with Croatel, d.o.o, and Geolux, d.o.o, Zagreb

• Innovative tracking system– in collaboration with Department of

Aeronautical Engineering at the Faculty of Mechanical Engineering and Nautical Architectures in Zagreb

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Tertiary payloads: Space-readiness of PureB detectors

• PureB detectors are detectors for electrons and ultra-violet light and are made using nanometer thin boron layer on silicon (nanotechnology)

• Technology has been developed at the University Twente/NL and in , detector developed in collaboration with FER/Zagreb.

– Detectors are commercially used in scanning electron microscopes.

Question: Can we use PureB detectors to track the electron density in ionosphere and can we use them to track ozone holes?

The objective:

• Demonstrate a detection system for measuring electron density and ultra-violet light measurements in space.

• Use the data to add information to the study of sun’s activity

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Ultra-violet light and electron-density detectionThe challenge:

• PureB has not been used for electron-density measurements in space at low electron density range (Ionosphere at 500 km has TE ~ 1400 K).

The approach

• Develop a practical detection system using PureB detectors

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energy harvesting

attitude control

control software

communicationelectronics

sensor data acquisitonelectronics

image and signal processing

Satellite build is a STUDENT project

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CubeSat development team

plus 50 students


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