Inquiry Question 2: What is the impact of changing technology on the development of new ideas?
Investigate limitations of current scientific instrumentation and how these have constrained scientific inquiry, with reference to a specific field such as genetics or astronomy
A focused answer to the HSC Investigating Science Module 6 dot point on limitations of technology. Covers how the resolution, sensitivity and cost of instruments constrain scientific inquiry, with worked HSC past exam questions using DNA sequencing and astronomy.
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What this dot point is asking
NESA wants you to identify how current scientific instrumentation limits the questions that can be asked, with named examples from specific fields. This dot point is about the mutual shaping of science and technology: technology limits science, and scientific breakthroughs open new technologies.
The answer
Every scientific instrument has limits: resolution, sensitivity, cost, accessibility, throughput. These limits shape which scientific questions can be asked and answered.
Categories of limitation
- Resolution
- The smallest detail an instrument can detect. A light microscope cannot resolve objects smaller than about 200 nm because of the wavelength of visible light. Atoms (about 0.1 nm) and viruses (10 to 100 nm) require electron microscopy.
- Sensitivity
- The lowest signal an instrument can detect. Detecting a single molecule of a hormone in blood requires extremely sensitive mass spectrometry or radioimmunoassay.
- Speed and throughput
- How fast measurements can be made. Sanger DNA sequencing (1977) reads 800 base pairs per day. Next-generation sequencing reads billions per day. The same scientific question, the same chemistry, but vastly different throughput.
- Cost
- Many instruments cost millions to billions of AUD. The Australian Synchrotron cost about 220 million AUD to build. The James Webb Space Telescope cost 10 billion USD. These constraints shape who can use them.
- Accessibility
- Even when instruments exist, access can be limited. Synchrotron beam time is allocated by peer-reviewed proposal, with success rates of about 30 per cent.
Field example: Genetics
The Human Genome Project (1990 to 2003) was a coordinated international effort to sequence the entire human genome. It cost approximately 3 billion USD and took 13 years.
The limitation. Sanger sequencing reads about 800 base pairs per reaction. Sequencing the 3 billion base-pair human genome required millions of reactions in parallel.
Cost trajectory.
| Year | Cost per genome |
|---|---|
| 2003 | 3 billion USD |
| 2007 | 1 million USD |
| 2014 | 1,000 USD |
| 2024 | Under 200 USD |
What changed. Next-generation sequencing (Illumina, Pacific Biosciences, Oxford Nanopore) parallelised the sequencing process across millions of microbeads or pores. Australia's Genomics initiative now sequences entire patient genomes routinely as part of clinical care.
What it enabled.
- Personalised medicine.
- Cancer genome characterisation.
- Pre-natal screening (non-invasive prenatal testing).
- Indigenous genome sequencing projects with First Nations consent.
- Pandemic surveillance (COVID-19 variant tracking).
Field example: Astronomy
- The limitation
- Earth's atmosphere absorbs many wavelengths and blurs ground-based images.
- Pre-1990
- Ground-based optical telescopes could resolve features about 1 arc-second across, limited by atmospheric turbulence. Infrared astronomy was nearly impossible from the ground because water vapour absorbs infrared.
- Solutions
- Space telescopes. Hubble (1990, optical and UV), JWST (2022, infrared), Chandra (1999, X-ray).
- Adaptive optics (1990s onwards). Deformable mirrors that correct atmospheric distortion in real time, reaching near-Hubble resolution from the ground.
- Radio telescopes (less affected by atmosphere). Australia operates the Murchison Widefield Array and the Australian Square Kilometre Array Pathfinder.
What it enabled.
- Discovery of exoplanet atmospheres.
- Hubble's measurement of the age of the universe.
- JWST's imaging of galaxies 13 billion years old.
- The first images of black hole event horizons (Event Horizon Telescope, 2019).
Field example: Microscopy
The limitation. Visible light has wavelengths around 400 to 700 nm. Diffraction prevents resolution of objects smaller than about 200 nm with standard light microscopy.
Solutions.
- Electron microscopy (1930s onwards). Electron wavelengths are about 100,000 times shorter than visible light, allowing resolution to atomic scale.
- Super-resolution microscopy (2000s). STED, PALM and STORM techniques exceed the diffraction limit by clever fluorescence methods. The 2014 Nobel Prize in Chemistry recognised this work.
- Cryo-electron microscopy (cryo-EM). Allows imaging of biological molecules in near-native states without crystallisation.
What it enabled.
- Structure determination of proteins and enzymes.
- COVID-19 spike protein structure (within weeks of the pandemic) using cryo-EM.
- Imaging of viruses and individual molecules.
Cost and access shaping research direction
When instruments are expensive, research direction concentrates around available capabilities.
- Australia's investment in OPAL, the Australian Synchrotron and the Pawsey Supercomputing Centre concentrates research in fields these instruments serve.
- Researchers in fields requiring instruments not available domestically must collaborate internationally or shift their research.
- The Australian Strategic Roadmap for Research Infrastructure (ASRRI) attempts to coordinate national investment.
When a limit is finally lifted
The history of science is full of moments when a technological breakthrough opened entire new fields:
- The microscope opened cell biology and microbiology.
- The telescope opened modern astronomy.
- Mass spectrometry opened modern chemistry and proteomics.
- DNA sequencing opened modern genetics.
- The Hubble Space Telescope opened modern cosmology.
Each breakthrough often follows decades of slow progress in the underlying technology, with the new science enabling the next round of technological advance.
Past exam questions, worked
Real questions from past NESA papers on this dot point, with our answer explainer.
2023 HSC6 marksUsing examples from at least two fields of science, explain how limitations of technology have constrained scientific inquiry.Show worked answer →
A 6-mark answer needs two distinct fields, the technological limitation in each, and the consequences for scientific knowledge.
- Field 1: Genetics
- Until the 2000s, DNA sequencing was slow and expensive. The Human Genome Project (1990 to 2003) cost approximately 3 billion USD and took 13 years to produce one human genome.
- Limitation
- Sanger sequencing (1977 method) could read about 800 base pairs per reaction. To sequence the 3 billion base-pair human genome required massive parallelisation and was financially prohibitive for most research.
- Consequence
- Genome-wide association studies, individualised medicine and large-scale comparative genomics were impossible. Most research focused on single genes.
- Breakthrough
- Next-generation sequencing (NGS) technologies (Illumina, Oxford Nanopore) developed from 2005 onwards reduced cost per genome to under 200 USD by 2024. The Australian Genomics initiative now sequences entire patient genomes routinely.
- Field 2: Astronomy
- Optical telescopes are limited by Earth's atmosphere. Atmospheric turbulence blurs images and water vapour absorbs infrared.
- Limitation
- Before the Hubble Space Telescope (launched 1990) and adaptive optics (1990s onwards), ground-based optical astronomy could not resolve fine detail in distant galaxies or detect very faint objects.
- Consequence
- The age of the universe, dark energy and exoplanet atmospheres were impossible to study.
- Breakthrough
- The James Webb Space Telescope (operational from 2022) sees infrared without atmospheric absorption, revealing the earliest galaxies and exoplanet atmospheres.
Markers reward two distinct fields, named technological limitations and the specific scientific questions opened by overcoming them.
2022 HSC4 marksExplain how the cost of scientific instrumentation can shape the direction of research.Show worked answer →
A 4-mark answer needs the cost mechanism, an example, and broader implications.
The mechanism. Cutting-edge instruments (synchrotrons, particle colliders, space telescopes, electron microscopes) cost tens of millions to billions of AUD. Only large institutions or international consortia can afford them. Research access is allocated competitively, and proposals must justify the instrument time.
Example. The Australian Synchrotron at Clayton (Melbourne) operates a particle accelerator producing intense X-ray beams. Access is allocated through peer-reviewed proposals. Researchers without competitive proposals or established credentials cannot use it.
Implications.
- Research direction. Funding pressures push research toward questions that can be answered with available instruments. Hypotheses that require new instruments are deferred.
- Concentration of expertise. Research becomes concentrated at institutions with access (Melbourne, Sydney, Brisbane, Canberra in Australia), disadvantaging regional universities.
- International dependence. Australia depends on overseas facilities for certain experiments (e.g. Antarctic ice-core analysis, particle physics at CERN). The Australian Strategic Roadmap for Research Infrastructure addresses this.
Markers reward the cost mechanism, a named instrument and at least two practical implications.
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