1. Introduction
Space missions—satellites, launch vehicles, interplanetary probes—require processors that are not just fast, but extremely reliable. Radiation, extreme temperature swings, long mission durations, and high cost of failure mean the architecture, fabrication process, and qualification are very different from consumer electronics. India’s recent unveiling of Vikram 3201 (also called Vikram-32) is a major move toward indigenous space-grade processing. To understand its place globally, it helps Vikram 3201 Comparison against established processors such as BAE’s RAD750, RAD5545, and those used by ESA (e.g. LEON / SPARC-V8 etc.).
Table of Contents
1. Introduction
2. Understanding the Requirements for Space-Grade Microprocessors
3. Vikram-32 / Vikram 3201 Comparison : Specs, Capabilities, and Design Goals
4. Overview of RAD750 and RAD5545 from BAE Systems
5. ESA / European Space Processors – LEON & SPARC lines
6. Side-by-Side Comparison: Key Parameters
7. What These Differences Mean in Real Missions
8. Strengths and Limitations of Vikram-3201 Compared to Others
9. Strategic Implications of India’s Entry into the Space-Processor Club
10.Conclusion

Vikram 3201 Comparison
2. Understanding the Requirements for Space-Grade Microprocessors
Before diving into specs, here are core requirements that distinguish space processors:
- Radiation hardness / tolerance (total ionizing dose, protection against single event upset (SEU), latch up, etc.)
- Operating temperature range (often −55°C to +125°C)
- Power consumption (since power is limited, especially beyond Earth or onnsatellites)
- Reliability & qualification: long lifetimes, robust packaging, fault detection, built-in test features
- Instruction Set, Floating Point Support, Real-time behavior: precise, deterministic operations, ability to support navigation / guidance / control algorithms.
- Fabrication technology node: older nodes (e.g. 180nm, 250nm) tend to be more mature and often more tolerant in high-radiation environments; trade-off against power, speed, density.
- These are the axes on which Vikram-3201, RAD750, RAD5545, etc., differ.
3. Vikram-32 / Vikram 3201 Comparison: Specs, Capabilities, and Design Goals
From published sources:
- Name / Identity: Vikram 3201, often called Vikram-32, developed by ISRO (Vikram Sarabhai Space Centre) in collaboration with Semiconductor Laboratory (SCL), Chandigarh.
- Fabrication process: 180 nm CMOS technology.
- Clock speed & supply / Power: ~100 MHz operation, single 3.3 V supply. Power consumption under ~500 mW; quiescent current <10 mA.
- Environment tolerance: Operates reliably in –55°C to +125°C.
- Instruction set / Language / Tools: Custom instruction set architecture (ISA)mtailored by ISRO. Supports floating-point computation. High-level languagem support: Ada is ready; C compiler is under development. Full in-house toolchain: compiler, assembler, linker, simulator, IDE.
- Other Functional Features: Dual on-chip MIL-STD-1553B bus interfaces; built-inmtest features (scan and functional modes). Packaging: 181-pin CPGA.
- Qualification / Deployment: Validated in space aboard the Mission Management Computer of the POEM-4 module during the PSLV-C60 mission. First production lots handed over as of early 2025.
So in summary, Vikram-3201 is India’s first fully indigenous 32-bit space processor, designed for launch vehicles and avionics, with a good balance of reliability, modest speed, and full local supply / toolchain.
4. Overview of RAD750 and RAD5545 from BAE Systems
RAD750
- A well-known radiation-hardened processor from BAE Systems (successor to RAD6000), based on the IBM PowerPC 750 architecture.
- Fabrication node: originally produced using 250 nm (also variants at 150 nm for certain hardened versions). Die area ~130 mm².
- Clock speeds: Between ~110 MHz to 200 MHz (depending on version).
- Performance: Can deliver ~266 MIPS and up; often extended with L2 caches.
- Radiation hardness: Very high tolerance; can survive large total ionizing doses (100,000 to more krad (Si)), wide temperature range.
- Power consumption: The processor itself consumes a few watts; systems (single‐ board computers) consume more (including memory, motherboards). For example, the RAD750 SBC can require ~10 W in some configurations.
RAD5545
- A more modern, higher performance processor from BAE Systems intended for newer missions.
- Performance: Reported spec: 64-bit Quad-core PowerPC, ~800 MHz, ~5200n DMIPS. Power consumption: Higher (~18-24 W) depending on mode.
- Better throughput, more modern interfaces: DDR3 memory, Flash, Serial RapidIO, SpaceWire, general purpose IO. Designed for SpaceVPX and modern avionics contexts.
5. ESA / European Space Processors – LEON & SPARC Lines
- While not alway a single product line, ESA / European designers (including Gaisler / Aeroflex / Cobham, etc.) have used SPARC-V8 / SPARC-V9 / LEON3 / LEON4 / LEON5 etc. for space applications. Some quick notable features:
- ESA’s LEON cores are open IP cores, radiation tolerant or hardened versions, often used in satellites, observatories, earth observation missions.
- These cores are usually in voltage and power regimes lower than RAD750 / RAD5545, but typically also lower peak performance; tradeoffs are made between redundancy, fault-tolerance, and power.
- Example: GR740 (Quad‐core LEON4-FT) rated ~250 MHz, with DMIPS in hundreds to low thousands, and power in a few Watts.s
- These ESA processor lines benchmark the mid-to-higher end (but often prioritize reliability, openness, toolchain maturity, and long mission support).
6. Side-by-Side Vikram 3201 Comparison: Key Parameters
Below is a table summarizing Vikram-3201, RAD750, and RAD5545 (and representative ESA processors) across key parameters:
Feature / Parameter | Vikram-3201 | RAD750 | RAD5545 | Typical ESA LEON / SPARC Processors |
Bit architecture | 32-bit, custom ISA | 32-bit PowerPC750 based | 64-bit, multi-core PowerPC | 32- or 64-bit SPARC / LEON cores |
Fabrication node | 180 nm CMOS | 250 nm (some 150 nm hardened variants) | M ore modern nodes, though still not bleeding edge CMOS │ ~180- 250 nm / older nodes; some hardened vnersions newer | – |
Clock speed | ~100 MHz | ~110-200 MHz | ~800 MHz (quad core) | ~200-300 MHz region for many designs |
Power consumption | < 500 mW (active), quiescent < 10 mA | Several watts to ~10 W for full board systems | ~18-24 W (for full systems) | Varies; ESA designs often few watts to low tens W depending on mission demands |
Temperature operating range | −55°C to +125°C | −55°C to +125°C | Similar or slightly more constrained depending on setup | Similar; often includes wide temperature ranges |
Radiation hardness | Designed for launch vehicle conditions; qualification in harsh environments | Very high, proven in many deep space / planetary missions | Expected to be highly hardened with modern protections | Designed / qualified for radiation tolerance; tradeoffs in speed vs protection |
Floatingpoint / precision | Supports floating-point operations | Supports FP (depending on variant and with cache etc.) | Strong floating-point, higher compute power | Varies; many provide FP support; higher complexity may add size/power |
Toolchain, language support | Ada ready; C in development; full in-house toolchain | C / C++; support for various RTOS, legacy ecosystems | Modern development environments; often supports Linux, RTOS | Strong tool support; ESA ecosystem has mature open tools and IP core availability |
7. What These Differences Mean in Real Missions
Understanding the spec differences is helpful, but what do they mean in terms of mission capability, cost, and reliability?
- Trajectory, Guidance, and Control Precision: Floating-point support and higher computational throughput (as in RAD5545) allow more complex algorithms (e.g. real-time correction, advanced control, path planning). Vikram-3201’s FP capability increases precision over older 16-bit units.
- Thermal & Environmental Reliability: Both RAD750 and Vikram-3201 are designed to survive extreme temperatures and radiation. Missions beyond low Earth orbit or with high exposure require high radiation hardness.
- Power and Size Constraints: Lower power consumption is vital. While RAD5545 offers higher speed, it comes at higher power cost; for many missions, especially smaller satellites or launch vehicle avionics, Vikram-3201’s lower power / moderate speed is acceptable or even desirable.
- Cost and Sovereignty: Procuring foreign processors (especially those hardened and flown) is expensive, with long lead-times, possible export controls. Vikram3201’s key advantage is being “Made in India”, including toolchains, packaging, qualification. This reduces dependency and can speed up mission design cycles.
- Mission Lifetime / Faults: Radiation induced faults can accumulate. Processors hardened through design, packaging, qualification, and long in-orbit testing (e.g. RAD750 has decades of flight heritage) offer proven reliability. Vikram-3201 has been validated in one mission so far; over time, more mission data will build trust.
8. Strengths and Limitations of Vikram-3201 Compared to Others Strengths
- Indigenous Design & Fabrication: Complete local supply chain for the chip, qualification, and tools. This is a strategic capability.
- Adequate for Many Space / Launch Vehicle Needs: For avionics, mission control, navigation, etc., 100 MHz, FP support, 1553B buses etc. are usable.
- Lower Power Footprint Compared to High-end RAD5545: More suitable for applications where power is constrained.
- Good Environmental Tolerance: Wide temperature range, built for “harsh” environments like launch vehicles.
Vikram 3201 Comparison Limitations / Areas for Growth
Lower Peak Throughput: Compared to RAD5545 (~800 MHz, quad-core etc.),Vikram-3201 is modest. For missions that need heavy image processing, massive data throughput (e.g. Earth observation with on-board compute, advanced autonomy), higher compute power may be needed.
- Radiation Hardness / Heritage: Though designed and qualified, the flight heritage is early. RAD750 has proven decades of flight use, many missions. Trust builds over repeated missions.
- NBTI, Aging, Single Event Effects etc. Smaller CMOS nodes often have more susceptibility; although 180nm is more mature, protections are still needed.
- Toolchain Maturity: Ada support is ready; C under development. For wider adoption, multiple languages, long-term maintenance, verification, etc., will need growth.
- Scalability for Multi-core / Parallel Architecture: Modern RAD5545 or ESA processors may offer multi-core or advanced SoCs. Vikram-3201 is single-core, fixed ISA; scaling performance upwards will require more cores or accelerators (FPGA, etc.).
9. Strategic Implications of India’s Entry into the Space-Processor Club
- Autonomy and Geopolitical Advantage: With supply chain fragility, export controls, sanctions, having indigenous space-grade processors means less dependence.
- Cost Savings & Faster Mission Turnaround: By designing, qualifying, and fabricating locally, ISRO may reduce cost, lead time.
- Enabler of New Missions: Smaller satellites, more frequent launches, satellite constellations, etc.,require more processors; a local processor eases scaling.
- Ecosystem Growth: Toolchains, software, packaging, qualification labs—all benefit local industry, academia, and defense.
- Benchmarking for Future Upgrades: Vikram-3201 is likely a base; future generations could include multi-core, more robust radiation hardness, faster nodes, heterogeneous architectures (accelerators, AI, etc.).
Vikram-3201 (Vikram-32) is a milestone for India: a fully indigenous 32-bit space-grade processor with floating-point support, designed in a mature fabrication node (180 nm CMOS), with wide environmental tolerance, and in-house software tools. While it does not (yet) match the peak performance of processors like RAD5545, or the decades of flight heritage of RAD750, it holds its own in many mission profiles, especially in launch vehicle avionics, satellite control, and where reliability per watt matters more than raw speed. As more missions use Vikram-3201, its reliability will be proven, and future versions may push the envelope further. For now, India has joined the elite club of countries capable of designing and manufacturing space-qualified microprocessors, an achievement that enhances national self-reliance, capability, and credibility in the space domain.