Nature Astronomy, volume 9, issue 1, pages 36-44
The NewAthena mission concept in the context of the next decade of X-ray astronomy
Mike Cruise
1
,
M. Guainazzi
2
,
James Aird
3
,
F. J. Carrera
4
,
Elisa Costantini
5
,
Lia Corrales
6
,
Thomas Dauser
7
,
Dominique Eckert
8
,
F. Gastaldello
9
,
Hironori Matsumoto
10
,
Rachel A. Osten
11, 12
,
P.‐O. Petrucci
13
,
D. Porquet
14
,
Gabriel W. Pratt
15
,
N. Rea
16, 17
,
Thomas H. Reiprich
18
,
Aurora Simionescu
5
,
Daniele Spiga
19
,
E. Troja
20
3
University of Edinburgh Institute for Astronomy, Royal Observatory, Edinburgh, UK
7
Remeis-Observatory & ECAP, FAU Erlangen-Nürnberg, Bamberg, Germany
10
14
LAM, Aix Marseille University, CNRS, CNES, Marseille, France
15
AIM, Université Paris-Saclay, Université Paris Cité, CEA, CNRS, Gif-sur-Yvette, France
16
Institute of Space Sciences (ICE-CSIC), Barcelona, Spain
|
17
Institut d’Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
|
Publication type: Journal Article
Publication date: 2024-12-31
Journal:
Nature Astronomy
scimago Q1
wos Q1
SJR: 3.311
CiteScore: 19.5
Impact factor: 12.9
ISSN: 23973366
Abstract
Large X-ray observatories such as Chandra and XMM-Newton have been delivering scientific breakthroughs in research fields as diverse as our Solar System, the astrophysics of stars, stellar explosions and compact objects, accreting supermassive black holes, and large-scale structures traced by the hot plasma permeating and surrounding galaxy groups and clusters. The recently launched X-Ray Imaging and Spectroscopy Mission observatory is opening in earnest the new observational window of non-dispersive high-resolution spectroscopy. However, several questions remain open, such as the effect of the stellar radiation field on the habitability of nearby planets, the equation of state regulating matter in neutron stars, the origin and distribution of metals in the Universe, the processes driving the cosmological evolution of the baryons locked in the gravitational potential of dark matter and the impact of supermassive black hole growth on galaxy evolution, to mention just a few. Furthermore, X-ray astronomy has a key part to play in multimessenger astrophysics. Addressing these questions experimentally requires an order-of-magnitude leap in sensitivity, spectroscopy and survey capabilities with respect to existing X-ray observatories. This article succinctly summarizes the main areas where high-energy astrophysics is expected to contribute to our understanding of the Universe in the next decade and describes a new mission concept under study by the European Space Agency, the scientific community worldwide and two international partners (JAXA and NASA), designed to enable transformational discoveries: NewAthena. This concept inherits its basic payload design from a previous study carried out until 2022, Athena. This Perspective looks forwards to the next decade of X-ray astronomy, explaining how it will contribute to better understanding of the high-energy Universe. In this context, the authors describe the NewAthena mission, a concept led by the European Space Agency.
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