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September 5, 2024 Newsletter - SatNow

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Weekly Edition
Date: September 5, 2024
 
MUNICH NEW SPACE SUMMIT 2024
 
 
Featured Space and Satellite Products
Low Noise Block
17.8 to 19.3 GHz Ka-Band Low Noise Block Downconverter
Low Noise Block  from AmpliTech

The APT5-LNB-17801930-92K10-WR42 from AmpliTech is a Low Noise Block Downconverter that converts an input RF frequency from 17.8–19.3 GHz to output IF frequency from 920-2420 MHz. It has an input VSWR of 1.25:1 and an output VSWR of 1.3:1. The low noise block downconverter weighs 2 lbs and measures 5.5 x 2.5 x 2.5 inches with WR 42 waveguide and SMA female interfaces. It is suitable for smallsats, LEO, MEO, GEO, and portable/fixed Ka-Band teleport applications.
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Star Tracker
Star Tracker Optical Head for Small Satellite Missions
Star Tracker  from Sodern

The AURIGA-CP from Sodern is a Star Tracker with a slew rate of 0.3-3 deg/sec and has a bias of 0.017 deg. This star tracker requires an optical head supply voltage of 5 V and has a power consumption of 0.8-1.1 W. It features baffle protection for the optical head for direct sun and earth illumination and software integrated into the spacecraft processor. The AURIGA-CP has a lifetime of up to 10 years in LEO and 50 years of experiences with star trackers and is ideal for small satellites missions.
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Space Qualified Resistor
1-1000 Ohms Space-qualified Thick Film Resistor Networks
Space Qualified Resistor  from Vishay

The MSM08C from Vishay is a Space Qualified Resistor with a resistance range of 10 Ohms to 1 MOhms. It has a power rating of 0.2-1.32 W and uses thick film resistive elements. It has a dielectric strength of 200 V and a voltage coefficient of resistance of about 50 ppm. This MIL-PRF-83401 qualified resistor is compatible with automatic insertion equipment with a molded epoxy body with copper alloy and hot solder dipped terminations. It weighs 1.1 g and measures 4.95 x 8.89 mm (L x W).
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Gimbal
Electric Propulsion Thruster Gimbal Assemblies
Gimbal  from Moog

The Model-L 3 Phase from Moog is a Gimbal that can be configured for wide rotation on both axes with a total rotational range of +/- 36 degrees (X & Y axis). It features dual axis gimbal driven by rotary actuators for cross-axis positioning, a potentiometer for position telemetry. It provides vector-pointing capabilities for various propulsion thruster configurations including Xenon, Arc-jet, and NTO/MMH, and has successfully been used for orbit raising and station keeping of heavier payload satellites.
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SATCOM Amplifier System
1500 W C-Band Solid State Power Amplifier for SATCOM Applications
SATCOM Amplifier System  from Communications & Power Industries

The MPCD61500M from Communications & Power Industries is a SATCOM Amplifier System with a frequency range of 5.850-6.425 GHz. It has a spurious of -70 dBc and a maximum VSWR of 1.3:1. It requires a power supply of 180-264 VAC. It features a modular architecture and QuadMod SSPAs that consist of four identical, forced air cooling system and fully inter-changeable RF plug-in modules. The amplifier system weighs 115 Kg (RF unit) and measures 483 x 577 x 695 mm (W x H x D).
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Attach and Release Mechanism
Hold Down and Release Mechanism for Satellite Payloads
Attach and Release Mechanism  from Ensign-Bickford Aerospace & Defense Company (EBAD)

The 9106 from Ensign-Bickford Aerospace & Defense Company (EBAD) is an Attach and Release Mechanism with a proof load rating of 40000 N and a release load rating of 32000 N. It has a max. angular misalignment of 6° cone. The mechanism is ideal for applications such as antennas, reflectors, solar arrays, deployable radiators, booms, masts, scientific instruments, satellite and spacecraft deployments, missile payload separation, launch vehicles, and missile stage and fairing separation.
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MUNICH NEW SPACE SUMMIT 2024
MUNICH NEW SPACE SUMMIT 2024
MUNICH NEW SPACE SUMMIT 2024
The Munich New Space Summit serves as a vital platform for the convergence of experts, researchers, industry professionals, and policymakers to engage in discussions, share insights, and explore collaborations within the realm of commercial space exploration. The event encompasses diverse facets of New Space, including satellite development and initiatives driven by private companies and entrepreneurial endeavors. Click here to learn more.
Test Loop Translator
17.60-19.10 GHz Test Loop Translator for Satcom Applications
Test Loop Translator  from Jersey Microwave

The KATLT-276291-176191-N22 from Jersey Microwave is a Test Loop Translator with an input frequency range of 27.60-29.10 GHz and an output frequency range of 17.60-19.10 GHz. It has an LO frequency of 10 GHz and a minimum return loss of 18 dB. It has a maximum spurious of -30 dBm and an SSB phase noise of up to -120 dBc/Hz (1MHz). It has a weight of 15 lbs and is designed for testing the satellite comm. between the up and downlink in the same band or uplink to L-Band.
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Space Qualified RF Filter
29.510-29.746 GHz Space Qualified Bandpass Filter
Space Qualified RF Filter  from Mercury Systems

The E1507 from Mercury Systems is a Space Qualified RF Filter with a frequency range of 29510-29746 MHz and has a maximum insertion loss of 1.5 dB. It has a passband phase deviation of +/- 5° and has a maximum VSWR of 1.5:1. This space-qualified RF filter  has a rejection of 40-60 dB and features a cavity design. It has a mass of 0.1 lbs and measures a package size of 0.75 x 1.25 x 4.0 inches. The filter is ideal for applications such as satellite communications and test equipment.
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Space Qualified Optocoupler
4 Pin Miniature LCC Optocoupler
Space Qualified Optocoupler  from Micropac Industries

The 66095-003 from Micropac Industries is a Space Qualified Optocoupler with a forward voltage range of 0.7-1.7 V and a static reverse current of 100 nA. It has a collector-to-emitter breakdown voltage of 40 V. It features an infrared LED and a silicon phototransistor in a 4 pin hermetically sealed leadless chip carrier. This optocoupler is designed for applications such as the high density surface mount circuits, ground loop isolation, feedback controls and general purpose switching circuits.
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Low Noise Block
7.75 to 8.5 GHz X-Band Low Noise Block Downconverter
Low Noise Block  from Orbital Research

The LNBX-EO from Orbital Research is an X-Band Earth Observation Low Noise Block (LNB) Downconverter that converts an input RF frequency of 8.0-8.5 GHz and an IF frequency of 950-1450 MHz. It requires a DC supply of 12-26 V. This LNB has an IP67-rated Aluminium sealed enclosure which weighs 1130 g and measures 270 x 79 x 55 mm. It is ideal for remote sensing, optical imaging, radar imaging satellites, LEO & MEO Small Sats, and high-resolution satellite imagery applications.
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DC to DC Converter
50 W Radiation Hardened Isolated DC to DC Power Converter
DC to DC Converter  from Microchip Technology

The SA50-120-28S-A-H from Microchip Technology is a DC to DC Converter that converts a DC input voltage of 120 V and a DC output voltage of 28 V. It has a gain of 60 dB and has a P1dB value of 15 dBm. It has a radiation tolerance TID of greater than 100 krad (Si) and a SEE immunity of 82 MeV·cm2/mg. It has a low mass of 120 g and measures 3.055 x 2.055 x 0.5 inches. It is based on flight-proven technology with a high MTBF and is ideal for space and military applications.
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Satellite Beacon Receiver
940–2150 MHz L-Band Digital Beacon Tracking Receiver
Satellite Beacon Receiver  from Novella SatComs

The B350 Series from Novella SatComs is a Satellite Beacon Receiver with an input frequency range of 940–2150 MHz. It supports the remote control options that include RS232 or RS422/RS485 with a D-type 9P F connector, serial emulation over TCP/IP with an RJ45 connector, SNMP and HTTP over TCP/IP Ethernet with an RJ45 connector. The receiver requires a power supply of 115 V/230 V and is suitable for antenna tracking of NATO, Skynet, or DSCS military beacons.
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MUNICH NEW SPACE SUMMIT 2024
 
 
RF Amplifier
16 to 32 GHz Monolithic Low Noise RF Amplifier
RF Amplifier  from United Monolithic Semiconductors

The CHA2069-FAB from United Monolithic Semiconductors is a Space-Qualified RF Amplifier that operates from 16-32 GHz. It is proposed in leadless hermetic metal ceramic 6 x 6 mm² package and requires a power supply of 4.5V/55mA. It requires a DC supply of 3.3 V and a max. drain current of 75 mA. This RoHS-compliant amplifier is dedicated to space communications and is also well suited for a wide range of microwave and millimetre wave applications and systems.
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Magnetorquer
Z-axis Internal Magnetorquer for Attitude Control of Nano-Satellites
Magnetorquer  from GomSpace

The NanoTorque Z-axis Internal from GomSpace is a Magnetorquer that has a dipole moment 139 mAm2 and a temperature coefficient of 0.571 O/°C. It has a total dipole resistance of 148 Ohms and a supply voltage of 3.3-3.4 V. The magnetorquer is placed within the PC104 stack by placing the magnetic field vector points the same direction as the stack connector. The magnetorquer is used with a satellites ADCS and designed for nanosatellites.
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Space Qualified Inductor
46.2 µH Space Qualified SMD Power Inductor
Space Qualified Inductor  from Exxelia Technologies

The CCM 20 46K 1W from Exxelia Technologies is a Space Qualified Inductor with an inductance of 46.2 µH. It has an isolation resistance of greater than 1 GOhm. It features Epoxy transfer molding technology and a ferrite core external assembly with SMD package weighing 21 g. This surface-mount inductor is designed to withstand severe environments such as space, avionics, and New Space applications and is ideal for energy storage, filtering, and smoothing applications.
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Satellite Terminal
Ka-Wideband 1.15 m Ruggedized Maritime VSAT System
Satellite Terminal  from Orbit Communication Systems

The OceanTRx 4MIL Ka from Orbit Communication Systems is a Space-Qualified Satellite Terminal with a Ka-band transmit frequency range of 29-31.0 GHz. The terminal is designed and tested for the strictest MIL-STD-810G environmental conditions. The terminal is has an optional fast manual band swapping with multiple BUCs per system and provides reliable, high-capacity, long-range multiband communication to navy vessels under extreme conditions.
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