Location via proxy:   
[Report a bug]   [Manage cookies]                
Skip to content
Link Boxes row [FP-hero-links-sl1]

What is LISA?

“Observing Gravitational Waves in Space”
… sounds impressive, but how and …

“Observing Gravitational Waves in Space” – Concept, Roadmap, …


News

Lorem ipsum dolor sit amet, consectetur adipiscing elit, sed …


Conferences

Stay informed about upcoming Conferences, Workshops and Meetings


Open Positions

Jobs & More


Papers

Papers & Reviews

LISA – the Laser Interferometer Space Antenna

The Laser Interferometer Space Antenna (LISA) is a large-scale space mission designed to detect one of the most elusive phenomena in astronomy – gravitational waves. This space-borne Gravitational Wave Observatory will have an arm-length of 2.5 million km, compared to the few km’s of the ground-based observatories.

LISA will observe the entire universe and discover parts that are invisible by other means. It will enhance our knowledge about the beginning, evolution and structure of our universe. LISA will complement earth-bound gravitational wave and other astronomical observatories, and significantly enrich multimessenger astronomy.

ESA: LST Team selected
GW Definition Box 1
Explanation from a popular website (PH)

ESA has announced the members of its LISA Science Team (LST): 18 scientists were elected and appointed for the first term from 2024 to 2027. The role of the LST is to provide scientific advice during the development and operations of the LISA mission. The LST is co-chaired by the ESA and NASA Project Scientists and will support the ESA Project and Operations teams on all aspects related to the science return of the mission.
Find the LST here: https://www.cosmos.esa.int/web/lisa/lisa-science-team

ESA: LISA Science Team selected
Mission Section text intro
GW Definition Box 1
Explanation from a popular website (PH)
ESA gives go-ahead for flagship gravitational-wave observatory
in space

Following its adoption, the LISA mission advances to the construction phase

LISA, the Laser Interferometer Space Antenna, has passed a major review with flying colours; the entire concept – frop the definition of the overall mission and operations to the space hardware to be built – stood up to the intense scrutiny of ESA’s reviews. Now the space agency’s Science Programme Committee (SPC) has confirmed that LISA is sufficiently mature and that mission development can proceed as planned. LISA should go into orbit in the mid 2030’s.

Mission Section text intro
GW Definition Box 1
Explanation from a popular website (PH)
The red book is out – learn all about the LISA space mission

The red book is a comprehensive document which just got published with the LISA adoption. It describes the mission in its whole and is the result of the relentless effort of the LISA Science Study Team.

Gravitational Waves – Technology – Data Analysis

The science as a foundation – the technology to make it happen – the data analysis to process the mission’s research data:

INDEX
Be in space to answer questions
Gravitational Wave Science
A New Astronomy
Features & Designs
Technology
What are LISA Sciencecraft
Methods and Tools
Data Analysis
Extracting Science

Gravitational waves encode information that isn’t accessible with light or particles. Combining these messengers will give us the power to understand the Universe in a whole new way.

Gravitational waves encode information that isn’t accessible with light or particles. Combining these messengers will give us the power to understand the Universe in a whole new way.

The classical distinction between spacecraft and payload doesn’t fit LISA well, because the LISA spacecraft are not just providing the infrastructure for the instruments. Each LISA spacecraft is part of the instrument itself because it protects the free-falling test masses from disturbances.

LISA leads to new methods and tools in data analysis. In preparing LISA data analysis experts met central challenges: they had to ensure that the LISA instrument will be able to deliver data relevant for scientific questions.

GW Sources – 2024

Cosmic Sources

LISA will be able to study gravitational waves generated by the following gravitational wave sources:

Cosmic fluctuations

Compact object falling onto a supermassive Black Hole

Merging intermediate Black Holes

Merging white Dwarfs in our galaxy

Merging supermassive Black Holes

Cosmic fluctuations in the early Universe

0%
1 Hz  
0%
10-4 Hz
0%
10-8 Hz
0%
 
0%
seconds
0%
hours
0%
years
0%