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First Direct Image of a Black Hole
Paul Ho, EAO/ASIAA
• E
BLACK HOLE SHADOW: APRIL 10, 2019
Breakthrough Prize, Einstein Prize, NSF Diamond Award, CTCI Award,…
Why is This Result Important ?
because it’s a real picture !
• Black Hole: “INVISIBLE” or “UNSEEABLE”
• Black Hole: where “GRAVITY” is strongest
• Black Hole: no escape — not even light
• Black Hole: no information from inside
• Small Black Hole: “end state” of big stars (>5-10 times sun)
— leftover after “supernova” explosion
• Big Black Hole: Billions times the sun’s mass
— in the nucleus of galaxies
• Black Hole Properties: high temperature? high density?
— depends on mass of Black Hole
• Black Hole Physics: tests General Relativity
• This Experiment is an “Optics” + “Information” Problem
What does the Image Say?
42μas
It’s Black, and Looks like a Hole
Recent BLACK HOLE Research
— Hear it, Feel it, (Not) See it
• Detection of Gravitational Waves (tens of cases)
• Progenitors of Gravitational Waves (one + )
• Orbital Motions at the Event Horizon (one)
• Imaging of the Event Horizon (two)
• GR Effects
• common technique: Interferometry
(optics and missing information problem)
Paul Ho, ASIAA/EAOGalaxy Forum 03.03.2020
LIGO ‘HEARD’ GW
• The LIGO experiment (another
interferometer) was designed to be
sensitive to the very ripples in space
caused by gravitational disturbances
• Like two black holes colliding…
GW Detectors: LIGO, VIRGO, KAGRA
Signatures of Gravitational Waves
Future GW Research
• Expanded Sensitivity and New Instruments
(Einstein Telescope, Cosmic Explorer, LISA)
• Many more detections, plus SMBHBs?
• Inspiral phase and post merger phase
• Theoretical Tests for GR effects
• Asia is invested in these future experiments
GRAVITY can be “FELT”
• The movement of stars - accelerated
to a fraction of the speed of light
around an invisible object - showed
SgrA* is likely a supermassive black
hole at the center of our galaxy
• Keck telescopes and GRAVITY
(VLT) have tracked them over 20
years (Andrea Ghez, Reinhard
Genzel)
GRAVITY collaboration+18a, A&A 615, L10
26 years of observations of S2
Stars in Orbit around SgrA*
ESO VLTI
Future Research of Dynamics
• Next Generation ISCO experiments
• extremely large telescope projects such as
TMT, ELT, GMT, can provide better
precision
• more accurate measurements of orbits
• fainter targets for orbital tests
• gas infall events detectable
• Asia is invested in these future experiments
GRAVITY can be “SEEN” ?
Take a Picture of Black Hole ?
• M87 black hole ~ 1 x 1043
g ~ 130 AU (Size)
• But M87 is very far! 53 Million Light Years
— 5 x 1020
km from us
• Schwarzschild Radius ~ 10 micro arcsecond
Sun or Moon ~ 30 arc minutes
M87 black hole ~ 5 x 10-9
size of moon
Spectrum vs Technology
submm ~ 10K 6000K
Problem Driven by Angular Resolution
Transparency
Precision
Energy
Scattering Extinction
• Mass will distort space-time until
even light cannot escape
• Einstein predicted the existence of
black holes - though even he was
n o t c o m f o r t a b l e w i t h t h e
conclusions from his equations
Gravity affects Geometry of Space
Gravity/Geometry instead of Material/Dielectric to bend Light
Shadow comes from General Relativity
Shadow Diameter ~ 5.2 Rsch
Artist's
im
pression!
VLBA 43 GHz VLA 20cm
VLA 15 GHz
60''
20''
5''
10mas
100µas
Image Credit: Bill Saxton NRAO/AUI/NSF
Walker et al (2008)
Zhou, Owen & Biretta
Case of M87
Directly Resolving the Black Hole
“because Seeing is Believing”
• Target Supermassive Black Hole
• Nearest Examples (SgrA*, M87)
(Shadow: ~5Rsch ~40 x 10-6 ’’)
• Very Long Baseline Interferometry
at Submm Wavelength
Precision ~ 10-10
Problem is Size
• The problem is nearby black holes are too small, and
supermassive black holes are too far. Existing
telescopes cannot resolve them.
• Two cases that look biggest to us would be at the
center of our galaxy… and one in M87 - 1000 times
further away, but also 1000 times bigger.
• The expected shadow around the black hole is just 50
µas
• We Need a telescope the size of the earth:
𝜃
array
= λ/D = 1.3mm/11000 km ~ 20 µas
DIFFRACTION PROBLEM
θ
Event Horizon Telescope in 2017
• Atacama Large Millimeter Array (ALMA), Chile
• ALMA Pathfinder Experiment (APEX), Chile
• James Clerk Maxwell Telescope (JCMT), Hawaii
• Large Millimeter Telescope (LMT), Mexico
• IRAM 30-meter Telescope, Spain
• South Pole Telescope (SPT), South Pole
• Submillimeter Array (SMA), Hawaii
• Submillimeter Telescope (SMT), Arizona
M.Johnson/SAO
JCMT is an EAO Initiative
Asia also working on SMA, ALMA, GLT
VLBI Experiment April 6, 2017
Aperture Synthesis: Building up UV Coverage
Visibility = Sampling . Source + Error
What does the Image Say?
42μas
Its Size, Brightness, Symmetry
Physical Parameters?
• Photon Ring: ~42µas or ~400au, round
• Schwarzschild radius: rs = 2 GM /c2
• Shadow Size ~5 times rs (Event Horizon radius)
—— as expected by General Relativity
—— deduced mass ~ 6.5 billion solar mass
• Ring Brightness: ne ~ 104 cm-3, B ~ 3G, Maccr ~ 10-3 Msun yr-1
• Ring Asymmetry: Brighter on Bottom Side
—— consistent with rotation with doppler boosting
• Tipped Disk: Perpendicular to Relativistic Jet
• Spin of Black Hole: Pointed away from Earth
Future Research in Imaging SMBH
• Galactic Center SgrA* Image is exciting
• M87 in 2018 has GLT data, which makes map “sharper”
• Polarization Data not yet fully analyzed
• AGN data were taken
• EHT experiment in 2020 will be much better:
GLT surface upgraded with improved efficiency
JCMT has new “GLT” receiver with 4x sensitivity
IRAM NOEMA will be available
• Asia will play a leading role in pushing Higher Resolution
!26
Summary 1
• Current Research depends on Angular Resolution
• Gravity Wave Research probes Coalescence Process in
building larger Black Holes
• Optical/IR Interferometry probes dynamics at Event Horizon
and test GR effects
• Submm Very Long Baseline Interferometry probes structures
of Event Horizon and physical processes and test GR effects
• Next Generation Instruments will have more resolution and
more sensitivity (time domain, energy domain, dynamics
domain)
• Asia will play a leading role in this Frontier in Optics/Physics!
!27
Summary 2
• Technology Greatly Improved: Materials, Instrumentation
• Technique Developed: VLBI and Computing
• ALMA Construction: Global Astronomy Mega Projects
• Nature Cooperated: “Enough” Accretion around Black Holes
• Hope: Refine and Test Physical Laws
Understand Universe and its Past and Future History
Stimulate Science for the Future
• Asia will and must play a leading role in this Adventure!
!28
East Asian Submm-VLBI Network
•  With	Tibet,	we	can	have	
East-Asian	Submm-VLBI	
Network	with	good	
imaging	capability	
•  Combine	with	North	
American	and	European	
telescopes,	it	is	possible	
to	have	Global	Submm	
VLBI	Network.
Greenland
Hawaii
Japan
Korea
Tibet
3C84
An EXAMPLE
EHT Telescopes 2017
!30
GLT in 2019

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Powehi EAO PPT from Director Paul Ho

  • 1. First Direct Image of a Black Hole Paul Ho, EAO/ASIAA
  • 2. • E BLACK HOLE SHADOW: APRIL 10, 2019 Breakthrough Prize, Einstein Prize, NSF Diamond Award, CTCI Award,…
  • 3. Why is This Result Important ? because it’s a real picture ! • Black Hole: “INVISIBLE” or “UNSEEABLE” • Black Hole: where “GRAVITY” is strongest • Black Hole: no escape — not even light • Black Hole: no information from inside • Small Black Hole: “end state” of big stars (>5-10 times sun) — leftover after “supernova” explosion • Big Black Hole: Billions times the sun’s mass — in the nucleus of galaxies • Black Hole Properties: high temperature? high density? — depends on mass of Black Hole • Black Hole Physics: tests General Relativity • This Experiment is an “Optics” + “Information” Problem
  • 4. What does the Image Say? 42μas It’s Black, and Looks like a Hole
  • 5. Recent BLACK HOLE Research — Hear it, Feel it, (Not) See it • Detection of Gravitational Waves (tens of cases) • Progenitors of Gravitational Waves (one + ) • Orbital Motions at the Event Horizon (one) • Imaging of the Event Horizon (two) • GR Effects • common technique: Interferometry (optics and missing information problem) Paul Ho, ASIAA/EAOGalaxy Forum 03.03.2020
  • 6. LIGO ‘HEARD’ GW • The LIGO experiment (another interferometer) was designed to be sensitive to the very ripples in space caused by gravitational disturbances • Like two black holes colliding…
  • 7. GW Detectors: LIGO, VIRGO, KAGRA
  • 9. Future GW Research • Expanded Sensitivity and New Instruments (Einstein Telescope, Cosmic Explorer, LISA) • Many more detections, plus SMBHBs? • Inspiral phase and post merger phase • Theoretical Tests for GR effects • Asia is invested in these future experiments
  • 10. GRAVITY can be “FELT” • The movement of stars - accelerated to a fraction of the speed of light around an invisible object - showed SgrA* is likely a supermassive black hole at the center of our galaxy • Keck telescopes and GRAVITY (VLT) have tracked them over 20 years (Andrea Ghez, Reinhard Genzel)
  • 11. GRAVITY collaboration+18a, A&A 615, L10 26 years of observations of S2 Stars in Orbit around SgrA*
  • 13. Future Research of Dynamics • Next Generation ISCO experiments • extremely large telescope projects such as TMT, ELT, GMT, can provide better precision • more accurate measurements of orbits • fainter targets for orbital tests • gas infall events detectable • Asia is invested in these future experiments
  • 14. GRAVITY can be “SEEN” ? Take a Picture of Black Hole ? • M87 black hole ~ 1 x 1043 g ~ 130 AU (Size) • But M87 is very far! 53 Million Light Years — 5 x 1020 km from us • Schwarzschild Radius ~ 10 micro arcsecond Sun or Moon ~ 30 arc minutes M87 black hole ~ 5 x 10-9 size of moon
  • 15. Spectrum vs Technology submm ~ 10K 6000K Problem Driven by Angular Resolution Transparency Precision Energy Scattering Extinction
  • 16. • Mass will distort space-time until even light cannot escape • Einstein predicted the existence of black holes - though even he was n o t c o m f o r t a b l e w i t h t h e conclusions from his equations Gravity affects Geometry of Space Gravity/Geometry instead of Material/Dielectric to bend Light
  • 17. Shadow comes from General Relativity Shadow Diameter ~ 5.2 Rsch
  • 18. Artist's im pression! VLBA 43 GHz VLA 20cm VLA 15 GHz 60'' 20'' 5'' 10mas 100µas Image Credit: Bill Saxton NRAO/AUI/NSF Walker et al (2008) Zhou, Owen & Biretta Case of M87
  • 19. Directly Resolving the Black Hole “because Seeing is Believing” • Target Supermassive Black Hole • Nearest Examples (SgrA*, M87) (Shadow: ~5Rsch ~40 x 10-6 ’’) • Very Long Baseline Interferometry at Submm Wavelength Precision ~ 10-10
  • 20. Problem is Size • The problem is nearby black holes are too small, and supermassive black holes are too far. Existing telescopes cannot resolve them. • Two cases that look biggest to us would be at the center of our galaxy… and one in M87 - 1000 times further away, but also 1000 times bigger. • The expected shadow around the black hole is just 50 µas • We Need a telescope the size of the earth: 𝜃 array = λ/D = 1.3mm/11000 km ~ 20 µas DIFFRACTION PROBLEM θ
  • 21. Event Horizon Telescope in 2017 • Atacama Large Millimeter Array (ALMA), Chile • ALMA Pathfinder Experiment (APEX), Chile • James Clerk Maxwell Telescope (JCMT), Hawaii • Large Millimeter Telescope (LMT), Mexico • IRAM 30-meter Telescope, Spain • South Pole Telescope (SPT), South Pole • Submillimeter Array (SMA), Hawaii • Submillimeter Telescope (SMT), Arizona M.Johnson/SAO JCMT is an EAO Initiative Asia also working on SMA, ALMA, GLT
  • 23. Aperture Synthesis: Building up UV Coverage Visibility = Sampling . Source + Error
  • 24. What does the Image Say? 42μas Its Size, Brightness, Symmetry
  • 25. Physical Parameters? • Photon Ring: ~42µas or ~400au, round • Schwarzschild radius: rs = 2 GM /c2 • Shadow Size ~5 times rs (Event Horizon radius) —— as expected by General Relativity —— deduced mass ~ 6.5 billion solar mass • Ring Brightness: ne ~ 104 cm-3, B ~ 3G, Maccr ~ 10-3 Msun yr-1 • Ring Asymmetry: Brighter on Bottom Side —— consistent with rotation with doppler boosting • Tipped Disk: Perpendicular to Relativistic Jet • Spin of Black Hole: Pointed away from Earth
  • 26. Future Research in Imaging SMBH • Galactic Center SgrA* Image is exciting • M87 in 2018 has GLT data, which makes map “sharper” • Polarization Data not yet fully analyzed • AGN data were taken • EHT experiment in 2020 will be much better: GLT surface upgraded with improved efficiency JCMT has new “GLT” receiver with 4x sensitivity IRAM NOEMA will be available • Asia will play a leading role in pushing Higher Resolution !26
  • 27. Summary 1 • Current Research depends on Angular Resolution • Gravity Wave Research probes Coalescence Process in building larger Black Holes • Optical/IR Interferometry probes dynamics at Event Horizon and test GR effects • Submm Very Long Baseline Interferometry probes structures of Event Horizon and physical processes and test GR effects • Next Generation Instruments will have more resolution and more sensitivity (time domain, energy domain, dynamics domain) • Asia will play a leading role in this Frontier in Optics/Physics! !27
  • 28. Summary 2 • Technology Greatly Improved: Materials, Instrumentation • Technique Developed: VLBI and Computing • ALMA Construction: Global Astronomy Mega Projects • Nature Cooperated: “Enough” Accretion around Black Holes • Hope: Refine and Test Physical Laws Understand Universe and its Past and Future History Stimulate Science for the Future • Asia will and must play a leading role in this Adventure! !28
  • 29. East Asian Submm-VLBI Network •  With Tibet, we can have East-Asian Submm-VLBI Network with good imaging capability •  Combine with North American and European telescopes, it is possible to have Global Submm VLBI Network. Greenland Hawaii Japan Korea Tibet 3C84 An EXAMPLE