Hubble Space Telescope – UPSC Notes

Hubble Space Telescope UPSC Notes | NASA–ESA | Legacy IAS Bangalore
Science & Technology · Space · UPSC GS-III

Hubble Space Telescope — NASA's Eye on the Universe 🔭

Complete UPSC Notes — How Hubble works, 6 scientific instruments, key discoveries (dark energy, age of the universe), one-gyro mode crisis (June 2024), Cloud-9 discovery (Jan 2026), Hubble vs JWST vs Roman comparison. Updated April 2026.

🚀 NASA + ESA Joint Mission Launched: Apr 24, 1990 ⚠️ One-Gyro Mode Since June 2024 35+ Years in Orbit Orbits at ~547 km (LEO) UV + Visible + Near-IR Wavelengths
📚 Legacy IAS — Civil Services Coaching, Bangalore  ·  Updated: April 2026
Section 01

🔥 10-Second Revision

📌 One-liner: The Hubble Space Telescope (HST) is a large space-based observatory — a joint NASA–ESA mission launched on April 24, 1990 aboard Space Shuttle Discovery. Named after astronomer Edwin Hubble. Orbits at ~547 km (Low Earth Orbit). Observes in UV, visible, and near-infrared wavelengths. Primary mirror: 2.4 metres. One of NASA's four "Great Observatories". Over 1 million observations and 22,000+ peer-reviewed papers. Shifted to one-gyro mode in June 2024. Expected to operate until 2030–2040.
1990
Year launched on Space Shuttle Discovery (STS-31)
547 km
Orbital altitude — Low Earth Orbit
2.4 m
Primary mirror diameter — same as Roman ST
1M+
Observations made · 22,000+ research papers
Section 02

🌍 Why Put a Telescope in Space?

Earth's atmosphere creates two fundamental problems for astronomers: (1) atmospheric turbulence makes stars "twinkle" and blurs images, and (2) the atmosphere blocks certain wavelengths of light completely (especially ultraviolet and parts of infrared). By placing Hubble above the atmosphere at 547 km, NASA eliminated both problems — giving Hubble a permanent, distortion-free, dark sky with no weather or light pollution.

📌 Key Advantage: Hubble can see objects 10× fainter than even the largest ground-based telescopes. It achieves extremely high angular resolution — distinguishing fine details in nebulae, galaxies, and star-forming regions that ground telescopes simply cannot resolve.
Section 03 — Must Know

⚙️ Scientific Instruments — 6 Key Systems

📷 WFC3
Wide Field Camera 3

Primary imager on Hubble. Records high-quality images in visible and ultraviolet light. Installed during the final servicing mission in 2009.

🔍 ACS
Advanced Camera for Surveys

Third-generation imaging camera optimised for broad surveys and wide-field imaging campaigns. Key for deep-field observations.

🌈 COS
Cosmic Origins Spectrograph

Focuses on ultraviolet (UV) light only. Best for studying bright point sources like quasars and stars. Analyses chemical composition of cosmic gas.

📊 STIS
Space Telescope Imaging Spectrograph

Second-generation spectrograph. Obtains high-resolution spectra across UV, visible, and IR wavelengths. Reveals chemical composition and temperature of objects.

🎯 FGS
Fine Guidance Sensor

Locks onto guide stars to provide precise pointing information. Three sensors work with gyroscopes and reaction wheels to keep Hubble steady during observations.

🔴 NICMOS
Near IR Camera & Multi-Object Spectrometer

Captures images and spectra at near-infrared wavelengths. Can peer through dust clouds to reveal hidden stars and structures.

📌 How Hubble Creates Colour Images: Hubble does NOT have colour cameras. It uses sensitive light detectors with special filters that allow specific colour ranges, creating black-and-white images. Scientists combine separate exposures through red, green, and blue filters (the three primary colours) to produce Hubble's famous full-colour images.
Section 04

🛰️ Hubble's Hardware & Support Systems

🪞 Primary Mirror
2.4 m diameter
🪞 Secondary Mirror
30.5 cm diameter
☀️ Solar Panels
GaAs Photovoltaic
📡 Antennas
2 × High-Gain
🔄 Gyroscopes
6 installed (2 functional)
🚀 Speed
~27,000 km/hr

Hubble's mirrors gather light from the cosmos; the secondary mirror reflects it back through a hole in the primary mirror into the instruments. An aperture door protects instruments from sunlight. Communication antennas beam data via NASA's relay satellites to the ground. Reaction wheels and gyroscopes control pointing. Solid-state recorders store data before transmission.

Section 05 — Important

⭐ Why Hubble Matters — Significance

🔍 Distortion-Free

Above atmosphere → no twinkling, blurring, or turbulence. Achieves higher angular resolution than any ground-based telescope of comparable size.

🌈 More Wavelengths

Sees UV and infrared wavelengths blocked by atmosphere. Reveals hidden details about chemical composition, temperature, and structure of cosmic objects.

🌑 Dark Skies

No light pollution, weather, or atmospheric interference. Permanent clear dark sky → sees objects 10× fainter than the largest ground telescopes.

🔧 Serviceable

Only space telescope designed to be serviced by astronauts — 5 shuttle missions repaired and upgraded instruments, optics, and gyroscopes.

🎯 Resolution

Extremely high angular resolution — distinguishes two closely-spaced objects. Captures fine details in star-forming nebulae, galaxies, and exoplanet atmospheres.

🔬 Diversity

Multiple instruments for imaging, spectroscopy, and interferometry. Spectrometers dissect light to reveal chemical composition and temperature.

Section 06

🌌 Major Discoveries

🕐 Age of the Universe

Pinpointed the age at ~13.8 billion years, narrowing it from a previous range of 10–20 billion years.

⚡ Dark Energy

Key role in discovering the mysterious force accelerating the universe's expansion. Contributed to the 2011 Nobel Prize in Physics.

🌀 Galaxy Evolution

Observed galaxies at every stage of evolution, including those from when the universe was still young — helping us understand how galaxies form.

🪐 Protoplanetary Disks

Discovered gas & dust disks around young stars — the birthplaces of new planets. Confirmed planet formation theory.

💥 Gamma-Ray Bursts

Revealed these mighty explosions occur in far-distant galaxies when massive stars collapse.

⭐ Earendel (2022)

Detected the most distant individual star ever observed — existing within the first billion years after the Big Bang.

Section 07 — Current Affairs 🆕

🔧 One-Gyro Mode Crisis (June 2024)

⚠️ Key Development: In June 2024, NASA permanently transitioned Hubble to one-gyroscope mode after one of its three remaining gyroscopes began returning faulty readings. This is a significant milestone in Hubble's ageing — and a potential UPSC question topic.

What are gyroscopes? Spinning wheels (at 19,200 RPM) that measure the telescope's orientation and rate of movement. Hubble originally had 6 gyroscopes (3 active + 3 spare), all replaced during the final servicing mission in 2009. By 2024, four had failed and one was giving faulty readings — leaving only two functional.

Gyroscope Status (2024–Present)
G1
Failed
G2
Failed
G3
Failed
G4
Faulty
G5
Reserve
G6
Active ✓

How does one-gyro mode work? The single active gyroscope is supplemented by other sensors — magnetometers (sense Earth's magnetic field), star trackers (use a map of the sky), and sun sensors — in a multi-stage process to achieve pointing accuracy nearly as good as the original three-gyro system.

📌 Impact: ~12% reduction in observing time and up to ~25% loss in scientific output. Cannot track fast-moving targets (Moon, inner solar system asteroids — but these were <1% of Hubble's observations). NASA estimates >70% chance of at least one functional gyro through 2035. No future servicing missions planned — Space Shuttle programme ended in 2011.

Feb 2026Novel Nanosatellite Solution Proposed 🆕

Researchers proposed deploying 4–6 nanosatellites on a tether ring around Hubble's body, each carrying compact gyroscopes, to restore motion-sensing ability without physically modifying the telescope. Estimated cost: under $10 million — compared to ~$900 million for the last shuttle servicing mission. The solution is reversible and upgradeable.

Section 08 — Current Affairs

🆕 Latest Discoveries (2025–2026)

Jan 2026"Cloud-9" — First Starless Dark Matter Cloud 🆕

Hubble discovered a new type of astronomical object — a gas-rich, starless cloud dominated entirely by dark matter, nicknamed "Cloud-9." Considered a relic of early galaxy formation — essentially a "failed galaxy". Furthers understanding of dark matter and galaxy formation.

Feb 2026CDG-2: Ghost Galaxy of 99% Dark Matter 🆕

Hubble identified Candidate Dark Galaxy-2 (CDG-2) — a galaxy almost entirely dominated by dark matter with only ~4 globular star clusters (vs Milky Way's 150+). Shines with the light of just ~1 million Suns.

Mar 2026Comet Breaking Apart in Real Time 🆕

Hubble accidentally captured comet C/2025 K1 (ATLAS) fragmenting into at least four pieces — the first time Hubble witnessed such an early-stage breakup. Analysis revealed the comet was unusually depleted in carbon. Published in Icarus.

Dec 2025First Witness to Planetary Collisions

Hubble witnessed catastrophic collisions of massive objects around the bright star Fomalhaut for the first time — similar to the dynamical upheaval our solar system experienced in its first few hundred million years.

Jun 2025Milky Way–Andromeda Collision Rethought

Using 10+ years of Hubble data, researchers found only a 50-50 chance of the Milky Way colliding with Andromeda within the next 10 billion years — challenging the previous consensus that collision was virtually certain.

Apr 202535th Anniversary Celebrated 🎂

Hubble celebrated 35 years in orbit (April 2025) with newly processed images of star clusters NGC 346 and Messier 72 using advanced data processing techniques.

Section 09

📅 Key Timeline

1946
Astronomer Lyman Spitzer publishes the concept of an extraterrestrial observatory
1990
Hubble launched aboard Space Shuttle Discovery (STS-31). Primary mirror flaw (spherical aberration) discovered
1993
STS-61 mission installs COSTAR corrective optics — Hubble begins delivering sharp images
1997–2009
Four more servicing missions; all five main instruments replaced/upgraded; 6 new gyros installed in 2009 (final mission, STS-125, Space Shuttle Atlantis)
2022
Detected Earendel — the most distant individual star ever observed
June 2024
Transitioned to one-gyro mode permanently; 4 of 6 gyros failed, 1 faulty
Apr 2025
Hubble celebrates 35 years in orbit
Jan 2026
Discovers "Cloud-9" — first confirmed starless dark-matter cloud / "failed galaxy"
2030–2040
Expected orbital decay and decommissioning (unless a reboost mission is undertaken)
Section 10 — Very Important

🔭 Hubble vs James Webb vs Roman — Comparison

🔭

Hubble Space Telescope

Launch
April 1990
Mirror
2.4 m
Wavelength
UV + Visible + Near-IR
Location
LEO (~547 km)
Field of View
Narrow
Serviced?
Yes — 5 missions
Agencies
NASA + ESA
Strength
UV vision; 35+ year legacy dataset
🌟

James Webb Space Telescope

Launch
Dec 25, 2021
Mirror
6.5 m (gold-coated, segmented)
Wavelength
Infrared (primarily)
Location
Sun-Earth L2 (~1.5M km)
Field of View
Wider than Hubble
Serviced?
No — too far away
Agencies
NASA + ESA + CSA
Strength
Sees through dust/gas; earliest galaxies
🛰️

Nancy Grace Roman ST

Launch
By May 2027
Mirror
2.4 m (same as Hubble)
Wavelength
Visible + Near-IR
Location
Sun-Earth L2 (~1.5M km)
Field of View
100× wider than Hubble
Serviced?
No
Agencies
NASA
Strength
Wide-area surveys; dark energy; exoplanets
📌 Exam Note — NASA's Great Observatories: Hubble is the visible light telescope in this programme. The others: Compton (gamma-ray), Chandra (X-ray), Spitzer (infrared). JWST is Hubble's infrared successor. Roman is Hubble's "wide-eyed cousin" — same mirror size but 100× wider field of view. Named after Nancy Grace Roman, NASA's first chief astronomer and the "Mother of Hubble."
🆕 Roman ST Update (Nov 2025): Construction completed at NASA's Goddard Space Flight Center. On track for launch on a SpaceX Falcon Heavy, possibly as early as late 2026. Its 288-megapixel Wide Field Instrument will gather data 100× faster than Hubble — adding 20 petabytes over its 5-year mission. A Coronagraph Instrument will directly image exoplanets by blocking starlight.
Section 11 — Practice

📝 UPSC-Style MCQs — Test Yourself

Q1Consider the following statements about the Hubble Space Telescope:
1. It was launched by the European Space Agency independently.
2. It orbits Earth at approximately 547 km altitude.
3. It can observe in ultraviolet, visible, and near-infrared wavelengths.

Which of the statements given above is/are correct?
a) 1 and 2 only
b) 2 and 3 only
c) 1 and 3 only
d) 1, 2 and 3
Hubble is a joint NASA–ESA mission (not ESA independently), making statement 1 incorrect. Statements 2 (547 km LEO) and 3 (UV + Visible + Near-IR) are correct. Answer: (b).
Q2Which of the following is NOT a feature unique to the Hubble Space Telescope compared to the James Webb Space Telescope?
a) It can be serviced by astronauts in orbit
b) It can observe in ultraviolet wavelengths
c) It is positioned at the Sun-Earth Lagrange Point 2
d) It orbits in Low Earth Orbit
JWST is at L2, not Hubble. Hubble orbits in LEO (~547 km). UV observation and in-orbit serviceability are unique Hubble features. Answer: (c).
Q3In 2024, NASA shifted the Hubble Space Telescope to "one-gyro mode." In this mode, what sensors supplement the single active gyroscope?

1. Magnetometers
2. Star trackers
3. Radar altimeters
4. Sun sensors

Select the correct answer:
a) 1, 2 and 3 only
b) 1, 2 and 4 only
c) 2, 3 and 4 only
d) 1, 2, 3 and 4
In one-gyro mode, Hubble uses magnetometers (Earth's magnetic field), star trackers (sky maps), and sun sensors along with the single gyro. Radar altimeters are not part of Hubble's pointing system. Answer: (b).
Q4Consider the following pairs:

Telescope → Primary Wavelength
1. Hubble → Infrared
2. James Webb → Infrared
3. Chandra → X-ray
4. Nancy Grace Roman → Visible + Near-IR

Which of the above pairs is/are correctly matched?
a) 1, 2 and 3 only
b) 2, 3 and 4 only
c) 1 and 4 only
d) 1, 2, 3 and 4
Hubble's primary wavelengths are UV + Visible + Near-IR (not primarily infrared), making pair 1 incorrect. JWST (infrared), Chandra (X-ray), and Roman (Visible + Near-IR) are all correctly matched. Answer: (b).
Section 12

🧠 Memory Aid — Quick Recall

🔑 Mnemonics & Key Facts for Exam Day

HUBBLE
High orbit (547 km) · Ultraviolet + visible + near-IR · Born 1990 (Shuttle Discovery) · Big mirror (2.4 m) · LEO position · ESA + NASA collaboration
GREAT 4
NASA's Great Observatories: Hubble (visible), Compton (gamma), Chandra (X-ray), Spitzer (IR)
13.8
Age of the universe determined by Hubble = 13.8 billion years
1 GYRO
June 2024 → one-gyro mode. 6 installed, 4 failed, 1 faulty, 1 active. Uses magnetometers + star trackers + sun sensors.
L2 TRIO
At Sun-Earth L2: JWST (2021) + Roman (2027). Hubble is in LEO — do NOT confuse.
ROMAN
Same mirror size as Hubble (2.4 m) but 100× wider field of view. Named after NASA's first chief astronomer. Launch by May 2027.
CLOUD-9
Jan 2026: First confirmed starless dark-matter cloud — a "failed galaxy" — discovered by Hubble.
Section 13

❓ Frequently Asked Questions

Why was Hubble's mirror initially defective?
Hubble's primary mirror was ground to the wrong shape due to a manufacturing error — a defect called spherical aberration. The mirror was too flat at the edges by just 2.2 micrometres (about 1/50th the thickness of a human hair). This tiny error caused light to focus incorrectly, producing blurry images. The problem was fixed in 1993 by installing the COSTAR (Corrective Optics Space Telescope Axial Replacement) system during the first servicing mission (STS-61). Later instruments had their own built-in corrective optics, making COSTAR obsolete.
Can Hubble still be repaired? Why not send another servicing mission?
The Space Shuttle programme was retired in 2011. All five servicing missions (1993, 1997, 1999, 2002, 2009) used the Space Shuttle's robotic arm and crew. No current crewed spacecraft has the capability to reach Hubble, grapple it, and allow astronauts to perform repairs. SpaceX and Jared Isaacman explored a concept to reboost Hubble's orbit (preventing re-entry), but NASA has not approved a servicing mission. In February 2026, researchers proposed a nanosatellite tether ring as a low-cost alternative to replace gyroscope functionality externally.
What is the difference between Hubble and JWST?
Key differences: (1) Wavelength — Hubble sees UV + visible + near-IR; JWST sees primarily infrared (can peer through dust/gas). (2) Mirror — Hubble's is 2.4 m; JWST's is 6.5 m (much larger collecting area). (3) Location — Hubble is in LEO (547 km); JWST is at Sun-Earth L2 (1.5 million km). (4) Serviceability — Hubble was serviced 5 times; JWST cannot be serviced. (5) Temperature — JWST has a sunshield keeping instruments at -233°C (essential for infrared observation). They are complementary, not replacements — Hubble remains the only space telescope with UV capability.
What is dark energy, and how did Hubble help discover it?
Dark energy is a mysterious force that constitutes roughly 68% of the total energy of the universe and causes the expansion of the universe to accelerate rather than slow down (as was expected due to gravity). In the late 1990s, two teams of astronomers used Hubble and ground-based telescopes to study distant Type Ia supernovae (exploding stars used as "standard candles" to measure cosmic distances). They found these supernovae were fainter than expected, meaning they were farther away — implying the universe's expansion was speeding up. This discovery earned the 2011 Nobel Prize in Physics. Hubble's sharp images were crucial for accurately measuring these distant supernovae.
What will happen to Hubble when it finally stops working?
Hubble's orbit is gradually decaying due to atmospheric drag (yes, there are trace amounts of atmosphere even at 547 km). Without a reboost, Hubble is expected to re-enter Earth's atmosphere between 2030 and 2040. NASA is considering options: (1) a controlled deorbit using an attached module to guide re-entry over the ocean, or (2) a reboost mission to raise its orbit and extend operations. A SpaceX/Polaris concept was studied but not approved. The telescope's instruments will likely fail before orbital decay forces re-entry.
Section 14 — Mains

📜 UPSC Mains — Probable Questions

📌 GS-III Paper: Science & Technology — Developments and their Applications. Space Technology. Awareness in the fields of Space.
Probable Question 1

"Discuss the significance of the Hubble Space Telescope in expanding our understanding of the universe. How has its successor, the James Webb Space Telescope, built upon Hubble's legacy?"

Probable Question 2

"Compare and contrast the Hubble Space Telescope, the James Webb Space Telescope, and the Nancy Grace Roman Space Telescope in terms of their design, capabilities, and scientific objectives."

Probable Question 3

"What are the challenges faced by ageing space infrastructure? Discuss with reference to the Hubble Space Telescope's gyroscope issues and proposed solutions."

Probable Question 4

"How have space telescopes contributed to our understanding of dark matter and dark energy? Discuss with suitable examples from the Hubble Space Telescope and the James Webb Space Telescope."

Section 15

🏁 Conclusion

🔭 Hubble — Humanity's Window to the Cosmos

For more than thirty-five years, Hubble has orbited 547 kilometres above Earth at 27,000 km/h, patiently collecting photons from the farthest corners of the observable universe. It arrived in orbit with a flawed mirror and was written off by critics. Then astronauts fixed it — and it rewrote the textbooks. The age of the universe. The existence of dark energy. The birth of stars and the death of galaxies. The first image of an exoplanet atmosphere. Each of these breakthroughs traces back, in part, to a single telescope circling above the clouds.

Today, Hubble operates on its last functional gyroscope — a spinning wheel smaller than a fist, turning at 19,200 revolutions per minute, holding one of humanity's greatest scientific instruments steady against the void. It is ageing, yes. But it is still discovering. In January 2026, it found Cloud-9, a dark-matter relic from the universe's infancy. In March 2026, it accidentally caught a comet tearing itself apart. Even in its twilight, Hubble keeps seeing things no one has seen before.

James Webb looks deeper into the infrared. Nancy Grace Roman will soon sweep the sky a hundred times wider. But neither can see ultraviolet light. Neither can be serviced by human hands. And neither carries thirty-five years of continuous observation — a scientific legacy that will inform astronomy for centuries after the telescope itself has re-entered the atmosphere. Hubble did not just observe the universe. It changed the way humanity understood its place within it.

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