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Planetary nebula in the constellation Cygnus
MWP 1, or the Methuselah Nebula, is a large planetary nebula surrounding the X-ray source RX J2117.1+3412. MWP 1 was first noticed in 1987 by Alain Maury
MWP_1
X-ray binary in Cygnus containing a stellar black hole
Cygnus X-1 (abbreviated Cyg X-1) is a galactic X-ray source in the constellation Cygnus and was the first such source widely accepted to be a black hole
Cygnus_X-1
Exoplanet candidate orbiting KOI-5715
Astrophysical Journal Supplement Series. 225 (1): 9. arXiv:1606.01744. Bibcode:2016ApJS..225....9H. doi:10.3847/0067-0049/225/1/9. "Purpose of Kepler Objects of Interest
KOI-5715.01
Topics referred to by the same term
that extend the life span of the animal Methuselah Nebula, nickname for MWP 1, a large planetary nebula Methuselah (planet), nickname for PSR B1620-26
Methuselah_(disambiguation)
North Atlantic regional climate era, c. 950 - c. 1250
The Medieval Warm Period (MWP), also known as the Medieval Climate Optimum or the Medieval Climatic Anomaly, was a time of warm climate in the North Atlantic
Medieval_Warm_Period
Blue supergiant star in the constellation Cygnus
the night sky, with an apparent magnitude slightly varying between +1.21 and +1.29. Deneb is one of the vertices of the asterism known as the Summer
Deneb
G-type star in the constellation Cygnus
parameters in the discovery paper, the planet is a super-Earth, with a radius of 1.87+0.33 −0.22 R🜨, and a predicted mass of 4.16 Earths. It has an orbit of
Kepler-1638
Cloud of heated and ionized gas and dust in the constellation Cygnus
the custom of the day. The Veil Nebula is expanding at a velocity of about 1.5 million kilometers per hour. Using images taken by the Hubble Space Telescope
Veil_Nebula
Planetary nebula in the constellation Cygnus
Humason 1-2 (Hu 1-2) is a bipolar hourglass shaped planetary nebula. Hu 1-2 was discovered by astronomer Milton L. Humason in October 11, 1920. The distance
Humason_1-2
Constellation in the northern celestial hemisphere
largest stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion
Cygnus_(constellation)
H II region in the constellation of Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Pelican_Nebula
Open star cluster in the Cygnus constellation
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_7011
Dark nebula
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Barnard_147
Supernova remnant in the constellation of Cygnus
The Astrophysical Journal. 754 (1): L7. arXiv:1206.4367. Bibcode:2012ApJ...754L...7K. doi:10.1088/2041-8205/754/1/l7. S2CID 54850975. Sharpless Catalog
Cygnus_Loop
Emission nebula in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Crescent_Nebula
Galaxy in the constellations Cepheus & Cygnus
supergiant. SN 2008S (Type IIn-pec/LBV, mag. 17.6) was discovered by Ron Arbour on 1 February 2008. SN 2017eaw (Type II-P, mag. 12.8) was discovered by Patrick
NGC_6946
The Victor Valley College Solar Farm is a 1.26 MWp (1.02 MWAC) concentrator photovoltaics (CPV) power station in Victorville, California. Upon completion
Victor Valley College Solar Farm
Victor_Valley_College_Solar_Farm
Hot Jovian exoplanet orbiting KELT-9
inclined orbit a mere 0.03462 AU from KELT-9 with an orbital period of less than 1.5 days. KELT-9b is a relatively large giant planet at about 2.2 times the
KELT-9b
Emission nebula in Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Propeller_Nebula
Star in the constellation Cygnus
been measured, radial velocity observations have set an upper limit of 9.1 M🜨 as of 2023[update]. Kepler-22b is the source of the extraterrestrial signal
Kepler-22
Emission nebula in the constellation Cygnus
geographical nomenclature. They appear to have been ejected from the cluster around 1.5 million years ago. Pelican Nebula Cygnus Molecular Nebula Complex "NASA/IPAC
North_America_Nebula
Star cluster in the Cygnus constellation
Journal of the Korean Astronomical Society. 44 (1). arXiv:1108.2134. doi:10.5303/JKAS.2011.44.1.1. Seligman, Courtney. "NGC 7093". Celestial Atlas.
NGC_7093
Solar power station in California, US
The Newberry Springs CPV Power Plant is a 1.68 MWp (1.5 MWAC) concentrator photovoltaics (CPV) power station in Newberry Springs, California. It was built
Newberry Springs CPV Power Plant
Newberry_Springs_CPV_Power_Plant
Star in the constellation Cygnus
suggest that the mean mutual inclinations of the planetary orbits are about 1°, meaning the system is probably more coplanar (flatter) than the Solar System
Kepler-11
Binary star system in the Cygnus constellation
( 1 − e ) ⋅ a ≈ 44 {\displaystyle {\begin{matrix}r_{per}\ =\ (1\ -\ e)\cdot a\ \approx \ 44\end{matrix}}} AU At apoapsis: r a p = ( 1 +
61_Cygni
Variable star in the constellation Cygnus
interferometry, which when discovered had an angular separation of 13.0±0.1 mas from the primary. It is 4.3 magnitudes fainter than P Cygni. It has been
P_Cygni
Concentrator photovoltaics (CPV) power station in Yucaipa, California
The Crafton Hills College Solar Farm is a 1.61 MWp (1.30 MWAC) concentrator photovoltaics (CPV) power station in Yucaipa, California. It was built by
Crafton Hills College Solar Farm
Crafton_Hills_College_Solar_Farm
Gas giant orbiting Kepler-1625
mostly composed of hydrogen and helium. It has been estimated to be 11.4±1.5 times Earth's radius, approximately equal to that of the planet Jupiter
Kepler-1625b
G-type main-sequence star in the constellation Cygnus
10 K cooler than this). However, its star is 6 billion years old (roughly 1.5 billion years older than the Sun). Due to this, Kepler-452b is receiving
Kepler-452
Star noted for unusual dimming events
Journal. 825 (1): 73. arXiv:1601.07314. Bibcode:2016ApJ...825...73H. doi:10.3847/0004-637X/825/1/73. S2CID 119211276. "TYC 3162-665-1". SIMBAD. Archived
Tabby's_Star
Nebula near the star Sadr
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
IC_1318
Planetary nebula in the constellation Cygnus
The Soap Bubble Nebula, Ju 1 (also known as PN G075.5+01.7) is a planetary nebula in the constellation Cygnus, near the Crescent Nebula (NGC 6888). The
Soap_Bubble_Nebula
Open cluster in the constellation Cygnus
background stars appear. Messier 29 can be found quite easily as it is about 1.7 degrees south of Gamma or 37 Cygni (Sadr). Angularly close, and almost certainly
Messier_29
Star in the constellation Cygnus
Spectral types at different phases of variation ranged from S6/1e to S9/1-e although no measurements were taken at minimum brightness. SiO masers were
Chi_Cygni
Exoplanet orbiting Kepler-16
the possibility of a habitable planet orbiting at a distance of about 0.95–1.02 AU, which could retain the thermal energy required to keep water in a liquid
Kepler-16b
Radio galaxy
M.K. (1953). "Fine Structure of the extra-terrestrial radio source Cygnus 1". Nature. 172 (4387): 996. Bibcode:1953Natur.172..996J. doi:10.1038/172996a0
Cygnus_A
Disappearing red supergiant star in the galaxy NGC 6946
nominal solar effective temperature of 5,772 K: ( 5772 / 3515 ) 4 ∗ 10 5.632 = 1 , 765 R ⊙ {\displaystyle {\sqrt {(5772/3515)^{4}*10^{5.632}}}=1,765\ R\odot
N6946-BH1
Series of German laws
900 MWp, feed-in tariff decreases 2.80 percent by more than 3,900 MWp, 2.50 percent, by more than 2,900 MWp, 2.20 percent, by more than 1,900 MWp, 1.80
German Renewable Energy Sources Act
German_Renewable_Energy_Sources_Act
Open cluster in the constellation Cygnus
September 2020. Segilman, Courtney. "Celestial Atlas". French, Sue (September 1, 2007). "The graceful swan: Cygnus is a wonderland for deep-sky observers"
IC_4996
Planetary nebula in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_6826
Double star system in the constellation Cygnus
consisting of β Cygni A (amber, apparent magnitude 3.1), and β Cygni B (blue-green, apparent magnitude 5.1). Separated by 35 seconds of arc, the two components
Albireo
photovoltaic modules of 450 MWp (2007: 210 MWp; 2006: 130 MWp) and with a production of 176 MWp (2007: 118 MWp; 2006: 84 MWp) Solon maintained to be one
Solon_SE
Red dwarf star in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Wolf_1069
Protoplanetary Nebula in the constellation of Cygnus
submicron-sized; on the other hand, dust grains in the circumstellar disk could be up to 1 mm. If the disk grains were micron-sized or smaller, it would be difficult
M1-92
Photovoltaic power station in Questa, New Mexico, USA
The Questa Solar Facility is a 1.17 MWp (1.0 MWAC) concentrator photovoltaics (CPV) power station in Questa, New Mexico. Upon its completion in late 2010
Questa_Solar_Facility
Binary star system in the constellation Cygnus
Astrophysical Journal Letters. 741 (1). L1. arXiv:1109.3198. Bibcode:2011ApJ...741L...1W. doi:10.1088/2041-8205/741/1/L1. "Kepler-16". SIMBAD. Centre de
Kepler-16
Star in the constellation of Cygnus
supernova. It is suspected to be a binary star with a companion orbiting about 1 au away. In 1966, a search for Wolf–Rayet stars in the northern celestial
WR_142
Red dwarf star in the constellation Cygnus
0.13 times that of the Sun, and a radius 0.17 times that of the Sun, just 1.7 times that of the gas giant Jupiter. Due to its small radius and hence surface
Kepler-42
Double-faced white dwarf star in the constellation Cygnus
Janus, also known by its name ZTF J203349.8+322901.1, is a transitioning white dwarf located more than 1,300 light-years (400 pc) away in the constellation
Janus_(star)
Reflection nebula in the constellation Cygnus
Clusters and Associations with Gaia DR2". The Astrophysical Journal. 870 (1): 32. arXiv:1807.02115. Bibcode:2019ApJ...870...32K. doi:10.3847/1538-4357/aaef8c
IC_5146
Planetary nebula in the constellation Cygnus
unusually small, measuring only 0.2 by 0.1 light-years, whereas the typical size for a planetary nebula is 1 light-year. It is fairly young, at about
NGC_7027
MWp Novoazovska wind farm [uk] - 107,5 MWp Krasnodon Wind Farm [uk] - 25 MWp Syvash wind farm [uk] - 246 MWp Orlivska Wind Power Plant [uk] - 100 MWp
List of power stations in Ukraine
List_of_power_stations_in_Ukraine
French renewable energy producer
solar plant (near Bordeaux, France), the largest of its kind in Europe (300 MWp) at the time of its commissioning in 2015; Mutkalampi, the largest wind farm
Neoen
Emission nebula in Cygnus constellation
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Sh_2-114
American water product manufacturer
Mueller Water Products, Inc. (MWP) is a publicly traded company headquartered in Atlanta, Georgia. It is one of the largest manufacturers and distributors
Mueller_Water_Products
Star cluster in the Cygnus constellation
Journal of the Korean Astronomical Society. 44 (1). arXiv:1108.2134. doi:10.5303/JKAS.2011.44.1.1. "Deep Sky Objects - NGC 7031 - open star cluster
NGC_7031
A-type main sequence star in the constellation Cygnus
averaged quadratic field of (194.5±230.7)×10−4 T. This star has a mass 1.67 to 1.75 times the mass of the Sun and is rotating with a projected rotational
29_Cygni
Triple star system in the constellation Cygnus
dwarf (B) and a cold brown dwarf of spectral type sdT8 (C). Wolf 1130 is 54.1 light-years (16.6 parsecs) distant from earth. The system is older than 10
Wolf_1130
Molecular cloud
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_6857
temperature record of the past 1000 years has improved. The Medieval Warm Period (MWP) and Little Ice Age (LIA) are the best-known temperature fluctuations in
Description of the Medieval Warm Period and Little Ice Age in IPCC reports
Description_of_the_Medieval_Warm_Period_and_Little_Ice_Age_in_IPCC_reports
Open cluster in the constellation Cygnus
cluster has an estimated mass of 232 M☉ and a linear tidal radius of 8.6±1.8 pc. Of the 15 brightest components, six form binary star systems; one more
Messier_39
Star in the constellation Cygnus
sized planets, in a general study of stars. Kepler-62 Gliese 667 TRAPPIST-1 Proxima Centauri b K-type main-sequence star Red dwarf Kepler-442 Barnard's
Kepler-186
Super Earth
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Kepler-371c
Emission nebula
velocity through space, forming a bow shock. The planetary nebula PK 87-3.1 is located within the nebula. and open cluster NGC 7044 is located nearby
Clamshell_Nebula
Star in the constellation Cygnus
in contrast with the earlier estimate from Barclay et al. (2013): 2.24 and 1.71 R🜨. Kepler-69c - a Venus-like exoplanet orbiting a Sun-like star List
Kepler-69
Gas giant exoplanet with a potential exomoon
slightly larger and more massive than the Sun, with a mass of 1.088±0.072 M☉ and radius of 1.117±0.064 R☉. It is also hotter and more luminous than the Sun
Kepler-1708b
Star in the constellation Cygnus
to be 1.15°. Stephen R. Kane did a dynamical analysis of the Kepler-89 system that demonstrated that planets c and d, although close to the 2:1 secular
Kepler-89
Star in the constellation Cygnus
Planets Encyclopaedia. Archived from the original on 19 January 2012. Retrieved 1 January 2012. Zacharias, N.; Finch, C.; Girard, T.; Hambly, N.; Wycoff, G
Kepler-70
Giant molecular cloud in the Milky Way
connected to one of the OB associations in the area, is the well-known Cygnus X-1 object, an X-ray source thought by many to be a black hole sucking matter
Cygnus Molecular Nebula Complex
Cygnus_Molecular_Nebula_Complex
Star in the constellation Cygnus
463. pp. 291–303. doi:10.1007/978-3-030-52144-8_13. ISBN 978-3-030-52143-1. Carter, J. A.; et al. (2012). "Kepler-36: A Pair of Planets with Neighboring
Kepler-36
Star cluster in the Cygnus constellation
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_7037
Solar power station in Haixi, Qinghai, China
270 acre 57.96 MWp Golmud 1 unit located 7 km south of the airport, and the 370 acre 79.83 MWp Golmud 2 unit located about 27 km east. Golmud 1 consists of
Golmud_CPV_Solar_Park
Star in the constellation Cygnus
science, Astronomers' Observing Guides, Springer, p. 82, ISBN 0-387-09460-1. "NNSV 11886". International Variable Star Index. AAVSO. Retrieved 2026-04-17
Kappa_Cygni
Open cluster in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_7063
Microlensing event
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
Gaia16aye
Star in the constellation Cygnus
velocities". Contributi Osservatorio Astronomico di Padova in Asiago. 239 (1): 1. Bibcode:1970CoAsi.239....1B. Kunitzsch, Paul; Smart, Tim (2006). A Dictionary
Gamma_Cygni
Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv:astro-ph/0409579, Bibcode:2005A&A...430..165F, doi:10
List_of_stars_in_Cygnus
Triple star system in the constellation Cygnus
On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S. Vallenari, A.; et al. (Gaia collaboration) (2023)
31_Cygni
Venus-like exoplanet orbiting Kepler-1649
The Astrophysical Journal. 830 (1): 1. arXiv:1608.00620. Bibcode:2016ApJ...830....1K. doi:10.3847/0004-637X/830/1/1. ISSN 0004-637X. McDonald, Rebecca
Kepler-1649b
Star in the constellation Cygnus
orbit and are in a highly eccentric orbit, which put their distances from 1.1 astronomical units in apoapsis to 30.5 astronomical units in periapsis. Its
Epsilon_Cygni
Planetary nebula in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_7026
Earth-size exoplanet orbiting Kepler-1649
orbital period of roughly 19.53 days, has a mass 1.2x times that of Earth, and has a radius of around 1.02 times that of Earth. Based on its mass and radius
Kepler-1649c
Open cluster in the constellation Cygnus
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
NGC_6819
Sun-like star in the constellation Cygnus
yielding values of 7.1, 9.0 and 9.7 R🜨 respectively, while masses were measured using transit-timing variations, giving masses of 2.1, 4.0 and 7.6 M🜨 respectively
Kepler-51
Star in the constellation Cygnus
I Candidate Red Supergiants in Gaia DR2". The Astronomical Journal. 158 (1): 20. arXiv:1905.03744. Bibcode:2019AJ....158...20M. doi:10.3847/1538-3881/ab1cbd
AZ_Cygni
Nebula
in the Sh2-112 Filamentary Cloud Complex". The Astrophysical Journal. 939 (1): 46. arXiv:2209.09609. Bibcode:2022ApJ...939...46P. doi:10.3847/1538-4357/ac940f
Sh_2-112
Star in the constellation Cygnus
confirmed in 2012. The planets form a resonant chain, with orbital periods ratio 1:2:4, although 20% probability exists that these period ratios may be coincidental
Kepler-31
Blue hypergiant star
not for the dust extinction, the star would have a visual magnitude about 1.5, nearly as bright as Deneb (Alpha Cygni), but because of the dust the observed
Cygnus_OB2-12
Energy Office cancelled it. 1 2 3 4 5 6 7 8 9 10 11 MVM Group: More than 5 MWp: Felsőzsolca, Paks, Pécs, Visonta Less than 5 MWp: MET Power: Százhalombatta
Wind_power_in_Hungary
Contact binary star system
MKCLASS Code". The Astronomical Journal. 151 (1): 13. Bibcode:2016AJ....151...13G. doi:10.3847/0004-6256/151/1/13. Kinemuchi, Karen (2013-10-01). "To Pulsate
KIC_9832227
Hot Jupiter orbiting TrES-5
Abell 78 Ear Nebula Egg Nebula Humason 1-2 IRAS 19475+3119 IRAS 20068+4051 IRAS 20324+4057 Kronberger 61 M1-92 MWP 1 NGC 6826 NGC 6842 NGC 6881 NGC 6884
TrES-5b
Binary star in the constellation Cygnus
luminosities are typical for their kind, with a luminosities of around 84% and 1% of that of the solar luminosity, respectively. The apparent magnitude of
Kepler-47
Multiple star in the constellation Cygnus
parallaxes overlap). Using the parallax of the A component, the distance is 21.1 parsecs. The parallax of the B component corresponds to a distance of 21.2
16_Cygni
Completed a 14.5 MWp solar PV, wind, and BESS hybrid expansion at the Rio Tinto QMM Mineral Sands mine. Dominican Republic: Completed the 33.4 MWp Monte Plata
Soventix_GmbH
Dark nebula in the Cygnus constellation
Spitzer Space Telescope". The Astrophysical Journal Supplement Series. 154 (1): 396–401. arXiv:astro-ph/0406371. Bibcode:2004ApJS..154..396Y. doi:10.1086/422818
L1014
Star in the constellation of Cygnus
lines at 465.0 nm for WR 140. Separation between the two stars varies from 1.3 AU at periastron to 23.9 AU at apastron. WR 140 is listed as a Wolf–Rayet
WR_140
Planetary nebula in the constellation Cygnus
the Fetus Nebula, is a planetary nebula with a diameter of approximately 1 light-year located at a distance of 2800 light years in northern Cygnus. It
NGC_7008
Star and surrounding nebula
the TESS Prime Mission". The Astrophysical Journal Supplement Series. 268 (1): 4. arXiv:2208.11721. Bibcode:2023ApJS..268....4F. doi:10.3847/1538-4365/acdee5
44_Cygni
Super-Earth orbiting Kepler-1652
of the star and the amount of light blocked, Kepler-1652b has a radius of 1.60 R🜨, within the super-Earth range between the sizes of Earth and the ice
Kepler-1652b
Photovoltaic power station in Imperial County, California
Mount Signal Solar, also known as Imperial Valley Solar Project, is a 794 MWp (614 MWAC) photovoltaic power station west of Calexico, California, United
Mount_Signal_Solar
travel, tourism, insurance
MWP 1
MWP 1
MWP 1
MWP 1
MWP 1
MWP 1
MWP 1
MWP 1
MWP 1
travel, tourism, insurance