From Wikipedia, the free encyclopedia
Star in the constellation Aquarius
40 Aquarii
is a star in the
equatorial
constellation
of
Aquarius
.
40 Aquarii
is its
Flamsteed designation
; it was too faint to be included in the
Bright Star Catalogue
.
[9]
The brightness of this star is below the normal limit for visibility with the naked eye, having an
apparent visual magnitude
of 6.93.
[2]
Based upon
parallax measurements
, it is located about 726
light-years
(223
parsecs
) away from the Sun.
[1]
It is moving closer to the Earth with a heliocentric
radial velocity
of -3 km/s.
[5]
40 Aquarii is positioned near the
ecliptic
and thus is subject to
lunar occultations
.
[10]
The
stellar classification
for 40 Aquarii is G5 IV,
[3]
matching a
G-type
, yellow-hued
subgiant star
that has exhausted the supply of hydrogen at its core and has begun to
evolve
into a
giant
. It is around 100
[7]
million years old with 10
[1]
times the girth of the Sun. The star is radiating 154
[4]
times the
luminosity of the Sun
from its
photosphere
at an
effective temperature
of 5,355 K.
[7]
References
[
edit
]
- ^
a
b
c
d
e
f
Brown, A. G. A.
; et al. (Gaia collaboration) (August 2018).
"
Gaia
Data Release 2: Summary of the contents and survey properties"
.
Astronomy & Astrophysics
.
616
. A1.
arXiv
:
1804.09365
.
Bibcode
:
2018A&A...616A...1G
.
doi
:
10.1051/0004-6361/201833051
.
Gaia DR2 record for this source
at
VizieR
.
- ^
a
b
Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".
Astronomy and Astrophysics
.
355
: L27?L30.
Bibcode
:
2000A&A...355L..27H
.
- ^
a
b
Houk, N.; Smith-Moore, M. (1988). "Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume 4, Declinations -26°.0 to -12°.0".
Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars
.
4
.
Bibcode
:
1988mcts.book.....H
.
- ^
a
b
c
d
Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",
Astronomy Letters
,
38
(5): 331,
arXiv
:
1108.4971
,
Bibcode
:
2012AstL...38..331A
,
doi
:
10.1134/S1063773712050015
,
S2CID
119257644
.
- ^
a
b
Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".
Astronomy Letters
.
32
(11): 759?771.
arXiv
:
1606.08053
.
Bibcode
:
2006AstL...32..759G
.
doi
:
10.1134/S1063773706110065
.
S2CID
119231169
.
- ^
a
b
van Leeuwen, F. (2007).
"Validation of the new Hipparcos reduction"
.
Astronomy and Astrophysics
.
474
(2): 653?664.
arXiv
:
0708.1752
.
Bibcode
:
2007A&A...474..653V
.
doi
:
10.1051/0004-6361:20078357
.
S2CID
18759600
.
- ^
a
b
c
d
e
f
g
Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics",
Astronomy and Astrophysics
,
501
(3): 941?947,
arXiv
:
0811.3982
,
Bibcode
:
2009A&A...501..941H
,
doi
:
10.1051/0004-6361/200811191
,
S2CID
118577511
.
- ^
"* 40 Aqr"
.
SIMBAD
.
Centre de donnees astronomiques de Strasbourg
. Retrieved
7 August
2017
.
- ^
Bidelman, W. P. (1990). "Flamsteed stars not contained in the Yale "Catalogue of Bright Stars"
".
Bulletin d'Information du Centre de Donnees Stellaires
.
38
: 13.
Bibcode
:
1990BICDS..38...13B
.
- ^
Boehme, D. (1978). "Derivation of Angular Diameters of Stars from Lunar Occultations".
Astronomische Nachrichten
.
299
(5): 243.
Bibcode
:
1978AN....299..243B
.
doi
:
10.1002/asna.19782990505
.
See p. 256.